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wankelmuth · 6 months
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Hamburg, 2023
Photo: Roland Helbig
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ffhyxrtg · 1 year
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Phil Hellmuth Mengikat Rekor Dunia dengan Gelang slotdemo ke-10 Menang!
Setelah banyak antisipasi, kesabaran, dan bakat untuk mengetahui kapan dia berada di puncak permainannya, Phil Hellmuth telah memenangkan gelang slotdemo ke-10, dan sekarang berada di antara yang terbaik dari yang terbaik! Setelah bertarung melawan 754 pemain di turnamen WSOP No Limit Hold'em Rebuy, Phil Hellmuth menang lagi! Setelah pertempuran panjang melawan Juha Helppi, Phil memenangkan $631.863, bagiannya dari kumpulan hadiah $2.340.238 dalam acara tersebut, tetapi yang lebih penting lagi; dia sekarang terikat dengan Brunson dan Chan untuk gelang WSOP terbanyak. Phil tidak pernah merasa lebih baik tentang permainannya, dan memenangkan gelang ke-10 rekornya sebelum acara utama jelas merupakan pertanda akan datangnya hal-hal yang lebih baik.
UltimateBet.com dengan bangga mensponsori Camp Hellmuth tahun ini. Bergabunglah dengan Phil Hellmuth dan teman-teman mulai 11 – 13 Agustus untuk akhir pekan terakhir poker yang dikemas dengan seminar, turnamen, makanan enak, dan teman yang fantastis. UltimateBet akan diwakili dengan baik dengan kehadiran Antonio Esfandiari, Freddy Deeb, Shawn Rice, dan P0ker H0. Bergabunglah dengan mereka bersama dengan profesional hebat lainnya dan bawa game Anda ke level berikutnya.
Lihat Phil Hellmuth saat dia bergabung dengan co-host Dave Foley sebagai komentator untuk “Celebrity Poker Showdown”. Saat musim kedelapan dimulai, Phil akan bermain-main dengan selebritas seperti Jason Alexander - yang sebenarnya diajarkan Phil cara bermain poker - Christopher Meloni, Macy Grey, Fred Savage, dan Jennifer Tilly. Para selebritas akan bersaing untuk mendapatkan hadiah satu juta dolar yang akan disumbangkan ke badan amal Badai Katrina. Musim baru di Bravo dimulai pada hari Rabu 31 Mei pukul 21:00 ET/PT.
Jika Anda bertanya kepada Phil Hellmuth siapa pemain poker terbaik di planet ini, cukup aman untuk berasumsi bahwa dia akan mengatakan 'Phil Hellmuth'.
Sementara sebagian besar penggemar Phil Hellmuth setuju, setidaknya satu orang tidak setuju.
“Phil Hellmuth adalah keledai,” kata juara poker yang memproklamirkan diri, Bill Fillmaff. “Donk da donk donk donk.”
Menjadi pria sejati, Phil telah memilih untuk mengabaikan pukulan konstan Bill Fillmaff. Tapi Fillmaff sudah keterlaluan.
"Dia bertindak terlalu jauh," kata Hellmuth. “Penghinaannya adalah satu hal, tetapi ketika seorang pria mengaku sebagai guru poker dan ternyata dia bahkan tidak tahu cara memainkan permainan itu, Phil Hellmuth harus menempatkannya di tempatnya.”
“Phil dapat menempatkan saya di tempat saya,” kata Bill Fillmaff. "Dan tempatku akan menjadi tempat pertama."
Untuk menyaksikan kompetisi poker terbesar dalam sejarah segalanya
Phil telah mendapatkan ketenaran di arena selebritas dan sering ditemukan bergaul dengan superstar dari semua genre. Dia akan berada di rumah di Derby karena balapan ini secara tradisional memiliki daya tarik khusus bagi set selebriti. Peserta selebritas sebelumnya termasuk Jack Nicholson, Jessica Simpson, Elliott Gould, dan Sean "P Diddy" Combs. Orang kaya dan terkenal yang berbaur di antara kerumunan Derby Day menambahkan dimensi unik pada tontonan "Run for the Roses".
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twof · 2 years
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Berlin, 2003
Photo: Roland Helbig
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filternewsofficial · 3 years
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Tension till the HoLiCOW comes home
Tension till the HoLiCOW comes home
How do we know of its existence? Various observations suggest it—like certain gravitational effects that are not explained by visible objects. Galaxies spin, but some spin as if they contain much more matter than is visible. Imagine trying to whirl a stone on the end of a string, but there’s an invisible boulder hanging from the middle of the string. Stars emit light, and this light sometimes…
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kunalverma2000-blog · 4 years
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MARS CRATERS STUDY
After reviewing the materials . I have decided that I am interested in physical characteristics of the craters, specifically the diameter (DIAM_CIRCLE_IMAGE) and depth (DEPTH_RIMFLOOR_TOPOG). While the morphology category data (MORPHOLOGY_EJECTA_1 through 3) is interesting too. This data is not available for most craters listed in the data set. Additionally, the available data on morphology may prove difficult to interpret based on my existing knowledge. I have decided to restrict my personal codebook to the following variables taken from the list in the Mars Crater Codebook –
 SPECIFIC TOPIC OF INTEREST
- Is there an association between the width of the crater and the depth of the rim of the crater?
 CODE BOOK
 1. CRATER_ID :Crater ID for internal use, in light of the rigion of the planet (1/16ths), the "pass" under which the crater was recognized, and the request where in it was distinguished.
 2. LATITUDE_CIRCLE_IMAGE: Latitude from the derived center of a non-linear least-squares circle fit to the vertices selected to manually identify the crater rim (units are decimal degrees North).
3. LONGITUDE_CIRCLE_IMAGE: Longitude from the derived center of a non-linear least-squares circle fit to the vertices selected to manually identify the crater rim (units are decimal degrees East).
4. DIAM_CIRCLE_IMAGE: Diameter from a non-linear least-squares circle fit to the vertices selected to manually identify the crater rim (units are km).
5.  DEPTH_RIMFLOOR_TOPOG: Average elevation of each of the manually determined N points along (or inside) the crater rim (units are km).
o Depth Rim –‐ Points are selected as relative topographic highs under the assumption they are the least eroded so most original points along the rim.
o Depth Floor – Points were chosen as the lowest elevation that did not include visible embedded craters.
MORPHOLOGY_EJECTA_1: ejecta morphology classified.
MORPHOLOGY_EJECTA_2: the morphology of the layer(s) itself/themselves.
MORPHOLOGY_EJECTA_3: overall texture and/pr shape of some of the layer(s)/ejecta that are generally unique and deserve separate morphological classification.
 SECOND TOPIC TO EXPLOREASSOCIATION WITH ORIGINAL TOPIC
Is there an association between the width of the crater and the depth of the floor of the crater? In other words, is the depth of the floor of the crater dependent upon the diameter of the crater?
 SOME BASIC QUESTION ASSOCIATION WITH SECOND TOPIC
Additional questions to be investigated in this study include the following:
- Is there an association/relation between the area of craters (based on its latitude & longitude) and the number of craters?Is there grouping of craters or there is the distribution of craters normally distributed?
- Is there an association/relation between the width of the crater and the number of ejecta layers?
 I will concentrate on whether there is a relationship between crater diameter and depth  in kilometers. As a stretch objective, I will determine if there is a secondary association between the noted characterstics and the crater location. The last may not be conceivable in the accessible time. While there are a few Python libraries that handle area information — models incorporate GeographicLib, GeoPandas, and ArcPy — these libraries may require some acclimation to deal with the coordinate system specific to mars to Mars.
 Based on the literature review (below) my hypothesis is:
As rim slope is somewhat related to crater depth so I can hypothesize that crater diameter and depth do have a direct correlation to each other. The degree to which they are related remains unknown at this point until I begin analysis.
H1: It is theorized that there is a correlation between the diameter of a crater and the depth of a crater.
H0: Given a random sample set of craters, the depth of a crater on Mars is not dependent upon the diameter width of the crater when assessed at the 95% confidence level.
 LITRECTURE REVIEW(REFRENCES)
Data source: Google Scholar
Data Queries: cratering on mars, Mars Cratering depth, Mars Cratering size
Synopsis and literature review findings: There are many papers referencing cratering on Mars as well as a comparison of Mars cratering to Lunar cratering. Barlow, Hartmann, and Ivanov seem to be primary sources. Topics referenced focus on surface properties of craters such as diameter, location, and morphology.
Robbins, S. J. (2011), Planetary Surface Properties, Cratering Physics, and the Volcanic History of Mars from a New Global Martian Crater Database., Site: Stuart Robbins, Astro/Geophysicist on the Web, 1–239, address: http://about.sjrdesign.net/files/thesis/RobbinsThesis_LargeMB.pdf, codebook: https://d396qusza40orc.cloudfront.net/phoenixassets/data-management-visualization/Mars%20Crater%20Codebook.pdf, data set: https://d18ky98rnyall9.cloudfront.net/_b190b54e08fd8a7020b9f120015c2dab_marscrater_pds.csv?Expires=1505865600&Signature=hlpupZ1s7N3Wxc8zZTdoN5U7M6WZK~ogycatsSlGxj45JJg2eDW6xlGUl-DTSFWzjPBZOn3QSFHnZHsQnSrjKowRM7OZgctqX1iY4iTJV7pYKqXRhnBeDFJHwaLywKHLzlbK8bi5CKE5jX~xHxXfE~sGIzuOE4l1fnWliaoXAXA_&Key-Pair-Id=APKAJLTNE6QMUY6HBC5A
Barlow, N. G. (1988). Crater size-frequency distributions and a revised Martian relative chronology. Icarus, 75(2), 285-305.
Barlow, N. G., & Bradley, T. L. (1990). Martian impact craters: Correlations of ejecta and interior morphologies with diameter, latitude, and terrain. Icarus, 87(1), 156-179.
Barlow, N. G., Boyce, J. M., Costard, F. M., Craddock, R. A., Garvin, J. B., Sakimoto, S. E., … & Soderblom, L. A. (2000). Standardizing the nomenclature of Martian impact crater ejecta morphologies. Journal of Geophysical Research, 105(E11), 26-733.
Chapman, C. R. (1974). Cratering on Mars I. Cratering and obliteration history. Icarus, 22(3), 272-291.
Hartmann, W. K. (1966). Martian cratering. Icarus, 5(1), 565-576.
Hartmann, W. K., & Neukum, G. (2001). Cratering chronology and the evolution of Mars. In Chronology and evolution of Mars (pp. 165-194). Springer Netherlands.
Ivanov, B. A. (2001). Mars/Moon cratering rate ratio estimates. In Chronology and evolution of Mars (p
McEwen, A. S. (2003, July). Secondary cratering on Mars: Implications for age dating and surface properties. In Sixth International Conference on Mars (Vol. 1, p. 3268).
Nimmo, F., & Gilmore, M. S. (2001). Constraints on the depth of magnetized crust on Mars from impact craters. Journal of Geophysical Research: Planets, 106(E6), 12315-12323.
Werner, S. C., Ivanov, B. A., & Neukum, G. (2009). Theoretical analysis of secondary cratering on Mars and an image-based study on the Cerberus Plains. Icarus, 200(2), 406-417.
Aharonson, O., M. T. Zuber, and D. H. Rothman (2001), Statistics of Mars’ topography from the Mars Orbiter Laser Altimeter: Slopes, correlations, and physical Models, J. Geophys. Res., 106(E10), 23723–23735, doi:10.1029/2000JE001403.
The Martian impact cratering record, Strom, Robert G.; Croft, Steven K.; Barlow, Nadine G.
Martian cratering II: Asteroid impact history, William K. Hartmann
Cratering Chronology and the Evolution of Mars, William K. Hartmann; Gerhard Neukum
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AAS NOVA Cepheid Yourself: Confirming Tensions in the Hubble Expansion By Astrobites Hubble’s law tells us that all galaxies, stars and planets are moving away from each other, and the more distant the object, the faster it is moving away. We quantify this expansion as a speed per distance, which gives us a unit like km/s (speed) per megaparsec (distance). This value is known as the Hubble constant, or H0. The Hubble constant has been determined using various methods. However, two of these titan measurements disagree with each other in a way that astronomers deem significant. The first of the measurements comes from studying the oldest electromagnetic radiation in the universe — the cosmic microwave background (CMB). See this Astrobite for a detailed explanation of how we are able to do this. The most recent results from the CMB give us a Hubble constant of roughly 67 km/s/Mpc. The second measurement comes from using Type Ia supernovae as standard candles to calibrate distances to them (see this Astrobite for more). Essentially, by looking at these stars at various distances, we can correlate their distance with their apparent brightness. By assuming supernovae are dimmer proportional to their distance from us, we can measure the gradient of this correlation. Recent results put H0 at 73 km/s/Mpc. So, one of the most prominent problems in cosmology boils down to a 6 km/s/Mpc difference. Certainly, each of these measurements have their own subtleties but there are two main things to note: The Hubble-constant measurements using the CMB and Type Ia supernovae are independent. They do not rely on the same measurement technique, and therefore do not have any source of error in common. This makes it harder to dismiss the tension as something which comes from a shared, inaccurate measurement. The Hubble-constant measurement from the CMB uses data from the early universe, while the value obtained from supernovae is a late-time or local measurement. This could potentially be an interesting explanation for the tension. A New Addition Today’s authors stir the Hubble cauldron a bit more with 70 space-based observations of Cepheid variables in the Large Magellanic Cloud (LMC) from the Hubble Space Telescope. A Cepheid variable is a type of star that pulsates over some period of time. Astronomer Henrietta Swan Leavitt deduced that the rate of pulsation for these stars is correlated strongly with their luminosity (see this Astrobite for more on her work and legacy). Therefore, one can know the brightness of these stars simply by observing their pulsation rate (centre image). Consequently, one can determine the distance to these stars just by comparing their known luminosity to the apparent brightness. Much like supernovae, this makes Cepheid variables powerful probes of the local Hubble constant. Furthermore, by studying galaxies containing both Cepheid variables and type Ia supernovae, the Cepheid-derived distances can be used to calibrate the accuracy of supernovae-derived distances, creating a robust distance ladder, which gets us to H0. To ensure an accurate Hubble-constant measurement with Cepheid variables, various sources of uncertainty are considered by the authors. Among these are the differences in the telescope sensitivity to fainter, distant Cepheids compared to nearer ones, which can affect the measured brightness. Another source of error is the inclination of the LMC itself, which results in some Cepheids appearing closer or farther than average by a very small degree. After taking all sources into account, the total uncertainty in the distance measurement, and hence the Hubble constant, is 1.28%, which is the smallest error for any Cepheid-variable Hubble-constant measurement to date. So What’s the Tension Now? Combining the LMC distances with two other distance calibrators for better constraints, the authors quote a Hubble constant of 74.03 km/s/Mpc, which is in a staggering 4.4-σ tension with the CMB Hubble-constant measurement. This effectively means that the probability that the new measurement is genuine rather than a statistical fluke is above 99.999%, and therefore so is the discrepancy. Much has been said on the nature of the Hubble disagreement already, both on its nature and from pacifists looking to ease the tension (see examples here and here). More recently, gravitational waves have burst onto the scene with another independent measurement (though it is not statistically significant enough to fuel the flames just yet). New physics could hold the key to breaking this Hubble stalemate. For example, our universe could have a non-zero curvature, a time-dependent dark energy, or interacting dark matter. Today’s paper shows that the tension is as strong as ever, so we wait for more precise, independent measurements to help clarify the nature of our expanding universe. Title: Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond ΛCDM Authors: Jacob Lustig-Yaeger, Victoria Meadows, Guadalupe Tovar Mendoza, et al. First Author’s Institution: University of Washington Status: Published in ApJ Editor’s note: Astrobites is a graduate-student-run organization that digests astrophysical literature for undergraduate students. As part of the partnership between the AAS and astrobites, we occasionally repost astrobites content here at AAS Nova. We hope you enjoy this post from astrobites; the original will be viewable at astrobites.org once the site has been fully restored. About the author, Sunayana Bhargava: I’m a third year PhD student in the Astronomy Centre at the University of Sussex. I study galaxy clusters with X-ray and optical data to learn about cosmology and the properties of dark matter. TOP IMAGE....The Hubble Space Telescope's views of the Large Magellanic Cloud have allowed astronomers to measure precise distances to 70 variable stars, improving estimates of the Hubble constant. [ESA/NASA/Hubble] CENTRE IMAGE....Period-luminosity relation for the 70 Cepheid variable stars. The colours in the figure indicate the different wavelengths used for observing these Cepheids. The agreement in the slope tells us the P–L relation is not dependent on any particular wavelength. [Riess et al. 2019] LOWER IMAGE....Various measurements of the Hubble constant colour-coded by whether they use data from the early universe (blue) or the late universe (red). At the top are potential modifications to our current cosmological model which could resolve the current tension. [Riess et al. 2019]
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contentone3 · 2 years
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Buy Dental Instruments Online-Diadent Paper Points-Dentsply Sirona Online
In dental medical procedures, it is utilized regularly in systems including endodontic medical procedures by dental specialists and consequently, a wide scope of loupes is generally accessible with dental providers relocate specialists have been utilizing engines provided by dental hardware vendors for their viability and cost-adequacy. Buy Dental Instruments Online In the creators' experience, dental instrument providers sell dental miniature engines which are compelling just as modest when contrasted with those provided by dermatology instrument vendors.
Dentalmicromotors utilized by endodontists are further developed for follicular unite collecting as these machines also show force and RPM of the engine during cryo-treatment, encompassing typical skin should be ensured by cool injury and unintentional rankles. In this situation, dental clay can be utilized to cover the encompassing skin before cryotherapy to forestall the spread of fluid nitrogen and skin harm. a dermatologist rehearsing in New York, in Collaboration with altered controlled dental hardware for use in dermabrasion. Robbins likewise fostered the precious stone fraise, which is generally utilized even today for dermabrasion.
There are a couple of organizations on the planet that produce a paper that focuses on standard size and none standard size. Albeit the physical, mechanical, and biochemical properties of these cones are vital, there are not many examinations on this issue, and on the off chance that there is, they are not with regards to Iranian brands. The point of this study is to assess one of the main properties of paper focuses, which is water assimilation, in two Iranian brands and examination of the qualities with Diadent. In this exploratory study,300 cones are arbitrarily chosen: 5 sizes selected (20,25,30,35,40) among brands Diadent Paper Points from each size 20 cones were assessed.
Carbide burrs can be utilized for beneficiary site groundwork for epidermal join a medical procedure in stable vitiligo which is accessible in dental stores in different shapes and sizes. These can be connected to a dental micromotor. The creators utilize a dental handpiece as it delivers more force and doesn't warm up effectively in long methods. Jewel fraises utilized in dentistry can be utilized for debulking of the nail plates in instances of onychomycosis and other dermatological signs. Photography for record support, revealing, and checking the treatment result is commanded by most clinicians. With the progression of telephone cameras, it has become simple for specialists to keep photography records. Intraoral photography is a troublesome assignment as lighting is low, the center doesn't function admirably with the telephone and DSLR camera.
To assess the bacterial decrease accomplished by WaveOne Gold (Dentsply Sirona Endodontics, Ballaigues, Switzerland), Hyflex EDM (Coltene-Whaledent, Altstätten, Switzerland), and XP-endo Shaper (FKG Dentaire SA, La Chaux-de-Fonds, Switzerland) in trenches tainted with Enterococcus faecalis. Dentsply Sirona Online The invalid speculation (H0) was that there would be no distinction among the NiTi frameworks in diminishing the root channel bacterial burden.
Thus, dental mirrors help to picture and catch Intraoral regions like the hard sense of taste. Disinfection is the main perspective even in minor medical procedures. A good sanitization framework in a center is vital for any system. Autoclaves are of different sorts, nonetheless, the most ordinarily utilized autoclaves are pressure-cooker type. They are liked in many centers because of their minimal expense. Elective, corresponding, integrative, and comprehensive medical services are matters of public intrigue and incorporate oral and dental consideration items.
Each cone weighed when the inundation of 16 mm of it in refined water for 5 seconds. Contrasts in these qualities show how much water assimilation for everyone. For information examination, the Kruskal-Wallis test and the Mann-Whitney "U" were utilized. Results: how much water ingestion between the 3 brands at size 20 and 25 are not huge. In sizes 30 and 35 assimilation of water in Aryadent is more than Sinadent and Sinadent is more than Diadent. In size 40 there is no huge distinction between Sinadent and Aryadent however how much water retention of Diadent is less. The crowns of 100 single-established teeth were taken out leaving 12 mm of the roots.
The channels were molded utilizing Endo-Sequence records. Following instrumentation, 80 teeth were separated into four gatherings. The leftover 20 teeth were separated into two gatherings. The heap at which crack happened was recorded and measurably broken down utilizing Kruskal-Wallis single direction examination of change and Z-tests. Inside the impediments of this review, UniCore quartz fiber posts gave the most elevated obstruction. This strategy may explicitly be beneficial for teeth with the capture of advancement at beginning phases, as these teeth are more helpless to crack attributable to their unnecessarily frail dentinal dividers.
The underlying dry load of paper focuses was determined by electronic lab balance, then, at that point, paper focuses were brought into the trench. The last weight after drenching of paper focuses was determined and distinction was noted. This interaction proceeded until the channel became dry.
Inserts with remaining profound testing pocket profundity decreased minimal bone level or changed surfaces following careful treatment of peri-implantitis present with expanded danger for repeat/movement. 74 mandibular premolar teeth with straight and round root channels were chosen. 62 root channels were tainted with E. faecalis for a considerable length of time and exposed to a mechanical arrangement with one of three single-record NiTi rotational frameworks WaveOne Gold, Hyflex EDM, and XP (Endo Shaper).
Twelve non-debased root waterways were utilized as regrettable controls. Bacterial examples were gathered with sterile paper focuses Dentsply Sirona Endodontics when revolving instrumentation to measure the bacterial burden. Five roots from every instrumentation bunch were assessed geographically from the coronal, center, and apical thirds by SEM. The bacterial decrease was determined and dissected genuinely by the Kruskal-Wallis and Dunn post hoc tests, all at 5% importance. No breaks of WaveOne Gold responding instruments happened during root waterway arrangements acted in maxillary and mandibular molars with arches when utilized stringently as per the producer's proposals and applied in a solitary clinical case. --
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1/11/2018 :(
I never want to forget it, so I’m making a list of memories I can think of. I’m going through all 628 photos we texted to each other since we started to text and my own photo gallery and I can see exactly how everything progressed, but here’s a list of memories I want to remember:
- the night we met
- the excitement I felt the first time you texted me, I went screaming to all my friends before I replied and that same night I told Meghan I’d met a really good guy
- the first few times we hung out I would go tell Erin and Nikki how it was and one night I’d really wanted you to kiss me and you hadn’t and I told them and they laughed at me
- our first date when I went to the wrong restaurant and you ordered chicken that I could smell throughout the entire movie
- when you came to my house for the first time and played with baby Guwwy the whole time and my heart melted
- when you asked to be my boyfriend with Starbucks and we parked in the boonies in Laguna and the restaurant you wanted to go to wasn’t super nice so we found somewhere else
- when we went to my winter formal and you saw me at photos and just said “wow”
- I misspelled Dwight
- that time Drew texted me after you didn’t shoot well and he said that you told him, “at least I can go home and talk to Lauren”
- when I used to send you Bitmojis all the damn time
- when Parnia asked if she could take you to prom??? wtf
- when my Dad told me that you and Austin wanted to play golf together 
- when we almost broke up but THANK GOD we didn’t because we really had no idea how incredible we would become
- the first time exploring your room
- when I didn’t know what a certain baking tool was and your mom said she needed to tell people about that at my wedding...like she knew
- when we slaved over chicken parmesan
- when we ruined multiple cakes
- when you broke a spoon mixing something and I almost peed
- when I broke your pool hose
- when I made you let me beat the Just Dance high score to Hey Ya! in my navy lace bralette and pants
- when we played that video game in your room with me in my Calvin Klein bra pants only
- when we laid in your room reading your childhood stories about Kale and I laid on little Ryan for most of it
- sexual tension filled Sequence
- when you tried to teach me chess and I will always be terrible
- when I beat your sorry ass at Scrabble
- the night with your cousins...need I say more
- when we spent New years together playing the game I bought your family
- when you made a whole dinner for my birthday and we danced the night away to Sinatra
- the first time we sexted
- when we sexted super late while I was at Yale and then wrote those love letters to each other
- trying to break into your bathroom and each time you’d catch me in a big hug
- every sleepover we had when we literally couldn’t sleep just because we were so close to each other
- Hawaii. that’s all I’m going to say because best week ever. 
- CIF Finals and prom after, the after party too
- when you sat with me and watched my graduation video through my whole childhood and even you made your appearances
- when I put all those photos in Kat from Yale and we both had such dreams for that to happen
- THE CAT
- snakey snake and death/Cameron
- when Romeo bit me
- your homecoming football game...you loved me so damn much
- the eagle golf club head cover
- that Harry Potter symphony plus our marathon
- all our comments on our Instagram photos
- when your Instagram profile photo at one point was of you running...you don’t RUN
- all the times I went golfing with you and we had so much fun and I made everything more peaceful for you
- when your contact name used to be Ryan (catfish h0) Wilson
- Devin’s party aka the night you said you could see yourself marrying me
- your sock subscription
- our matching underwear and photos
- our home video
- roadhead
- yoghurt
- Andrea
- when autocorrect made you say “pussy” instead of pissy
- when we danced the night away at BOTH homecomings
- when we played hangman and used Xerox
- in November when we fought and Meghan had to tell us that we had something people would die for and to never forget that...
- when you gave me a freaking hickey on accident 
- your birthday when you sent me that message about “rebound girl my ass you’re an 11/10 how tf did I even score you”
- 3 under par kind of night
- 15 reasons you love me
- when you got into Harvard and we thought everything in KAT would come true
- when we went on that Ferris wheel the first time we hung out and you fell in love with my head twitch and the first time you touched my back to lead me off the ride I got chills all over
- when you said your name was Jamal at Starbucks and none of your gift cards worked but it was so perfect
- UCLA basketball game fun and your attempt to eat crab causing you to get a second dinner
- Disneyland!!
- all those times when you made me pancakes, especially when you’d wake up early for me if you didn’t have school and I’d get to start my day with you
- When you told me you loved every single fucking thing about me and that I’m the best girl to walk this planet and you were so lucky to meet me by chance
- Harvard/Yale meme sharing
- when you asked me to prom the day before with the greatest poster ever
- when you showed your mom the video from my signing day and she started crying because she was so proud
- when you came to my graduation and when I walked out I’m pretty sure I heard you yell “AYO” like you do
- when you were being all humble about your senior award so I stalked it and turns out it’s the best you can get
- when you’d hit me with those random appreciation notes about my booty or how much you love me
- your senior speech that puts me in tears with how good it is
- Hawaii deserves another mention
- when you looked at me on that last night in Hawaii and literally couldn’t even comprehend my beauty
- right before my Yale interview when you told me I was your inspiration
- our bow on my head naked fantasy (and all the other fantasies we had together)
- “girl get it”
- my second birth control reminder was “YOU LOVE RYAN”
- I once put a note in my phone under your contact that says “he loves me” in case I ever got amnesia or something and I think it’s still there
- Universal deserves all the mentions in the world honestly best day ever
- lobey dersh and rye bread wilsonian
- When I drove to your house at 4am to say goodbye
- when we got pizza after almost breaking up and I was so happy
- when we had a sleepover and you walked into me wearing all of your clothes
- I always wish for more, but these were the best two years of our lives with the people who made us happiest...to be continued one day, or to not
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natazaelia · 7 years
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When in doubt, put a ruler on it. DYO experiments... pǝɯɯɐɹƃoɹd sı ʎʇıןɐǝɹ ɹnoʎ Here's a resource to get you started: https://dizzib.github.io/earth/curve-calc/?d0=30&h0=6&unit=imperial #NASAlies #curve #fe #PLANE #earth #planeterra #planet #flatearth #eye #photo #opticalillusion #DOMELIFE #nasa #hoax #horizontal #ruler #photograph #picture #globe #world #skyline #test #diy #news #experiment #horizon #city #globe #boat #eyes #lighthouse
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wankelmuth · 6 months
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Hamburg, 2023
Photo: Roland Helbig
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naturegigs · 4 years
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Expansion of universe: mysterious things
An emergency in material science may have recently gotten further. By taking a gander at how the light from inaccessible splendid articles is bowed, scientists have expanded the inconsistency between various strategies for ascertaining the development pace of the universe.
"The estimations are reliable with demonstrating an emergency in cosmology," Geoff Chih-Fan Chen, a cosmologist at the University of California, Davis, said here during a news preparation on Wednesday (Jan. 8) at the 235th gathering of the American Astronomical Society in Honolulu.
At issue is a number known as the Hubble consistent. It was first determined by American cosmologist Edwin Hubble about a century prior, after he understood that each world known to mankind was zipping endlessly from Earth at a rate relative to that system's good ways from our planet.
This doesn't imply that Earth is at the focal point of the universe. Rather, the discovering told researchers that the universe is growing and that there is an immediate connection between how far separated two articles are and how quick they are subsiding from each other. The Hubble steady has a worth that consolidates this speed-separation association.
The issue is that, as of late, various groups have differ over what precisely this current steady's worth is. Estimations made utilizing the inestimable microwave foundation (CMB), a remainder from the Big Bang that gives a depiction of the baby universe, recommend that the Hubble consistent is 46,200 mph for every million light-years (or, utilizing cosmologists' units, 67.4 kilometers/second per megaparsec).
Be that as it may, by taking a gander at throbbing stars known as Cepheid factors, an alternate gathering of space experts has determined the Hubble steady to be 50,400 mph for every million light-years (73.4 km/s/Mpc).
The inconsistency appears to be little, yet there is no cover between the autonomous qualities and neither one of the sides has been happy to yield significant slip-ups in its procedure.
The new estimation, made by the H0 Lenses in COSMOGRAIL's Wellspring (H0LICOW) joint effort, was an endeavor to ascertain the Hubble consistent in a totally novel manner. (COSMOGRAIL is the abbreviation for Cosmological Monitoring of Gravitational Lenses.)
This measure utilizes the way that huge items known to man will twist the texture of room time, implying that light will twist as it goes past them. Superluminous, dark opening controlled elements called quasars are now and then discovered behind enormous frontal area worlds, and their light gets twisted by this bowing procedure, which is known as gravitational lensing.
Utilizing the Hubble Space Telescope, the H0LiCOW group contemplated the light from six quasars between 3 billion and 6.5 billion light-years from Earth. As the quasars' dark gaps ate material, their light would glimmer.
The interceding gravitationally lensing world twisted every quasar's light, thus the quasar's gleaming landed at Earth at various occasions relying upon what way it took around the frontal area cosmic system, Chen said. The length of the time defer gave an approach to test the extension pace of the universe, he included.
H0LiCOW had the option to determine an estimation of the Hubble consistent of 50,331 mph for each million light-years (73.3 km/s/Mpc), incredibly near that gave by Cepheid factors yet very a long way from the CMB estimation.
"The outcome is the strain is very well likely genuine," Chen said and presumably not the aftereffect of mistakes in the techniques for each approach.
It's significant that last year another free estimation of the Hubble consistent, made utilizing monster red stars, came soundly between the different sides, ascertaining an estimation of 47,300 mph for every million light-years (69.8 km/s/Mpc).
All things considered, Chen stated, the various numbers are far enough separated that it's conceivable there is something incorrectly in our models of the universe. A developing number of physicists are recognizing this, he included, in light of the fact that the free estimations keep on opposing this idea. Scientists may need to think of new material science to clarify what's happening.
Universe is a mystery  save earth, save future :)  #wedonthaveoption
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twof · 2 years
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Berlin, 2020- 2022
Photo: Roland Helbig
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THE BEST PERSONAL WATERCRAFT TO KEEP ON BOARD
1. Sea-Doo Spark Trixx
One for the daredevils, Sea-Doo's Spark Trixx has been designed to make impressive Jet Ski stunts easier and more fun that ever. A handlebar with adjustable riser allows you to customise the watercraft to your riding style while step wedges provide greater stability and control for stand-up riding and a variable trim system exaggerate how high you can raise the nose or how deep you can bury it making your tricks look better than ever. Powered by a Rotax 900 H0 ACE engine, the Spark Trixx also has an intelligent brake and reverse system and Sport and Touring acceleration modes so you get the perfect ride every time.
Sparedevil Sea-Doo Spark Trixx был разработан для того, чтобы делать впечатляющие трюки Jet Ski проще и веселее. Регулируемый руль позволяет вам настроить водный мотоцикл на свой стиль езды, в то время как шаговые клинья обеспечивают большую стабильность и контроль при стоячем езде, а переменная система отделки преувеличивает, насколько высока вы можете поднять нос или насколько глубоко вы можете делать трюки и выглядят лучше, чем когда-либо. При работе от двигателя Rotax 900 H0 ACE Spark Trixx также имеет интеллектуальную систему торможения и реверса, а также режимы ускорения спорта и туризма, поэтому вы получаете идеальную езду каждый раз.
2. Sea-Doo GTX Limited
The huge Rotax 1630 ACE engine puts out 300hp, controlled using the intelligent throttle. Sea-Doo’s unique braking technology also allows it to stop nearly 50m before other watercraft would. It features a removable three person seat.
Огромный двигатель Rotax 1630 ACE выпускает 300 л.с., управляемый с помощью интеллектуального дросселя. Уникальная технология торможения Sea-Doo также позволяет остановить почти 50 м до того, как будут использоваться другие суда. Он оснащен съемным трехместным сиденьем.
3. Kawasaki Ultra 310LX
Billed as the fastest jet ski on the planet, Kawasaki’s flagship model features a big 1,498cc engine, supercharged with Eaton Twin Vortices, Kawasaki’s flagship PWC packs a mighty punch – and it features Jetsound Bluetooth audio.
Флагманская модель Kawasaki, представленная как самые быстрые водные лыжи на планете, оснащена большим двигателем мощностью 1,498 куб. См, с наддувом с вихрями Eaton Twin, флагманской PWC от Kawasaki - мощный удар, а в нем есть звук Jetsound Bluetooth.
4. Yamaha GP1800
The GP1800 boasts incredibly tight cornering and stability in tougher conditions, as well as a top speed of 70mph thanks to a 1.8 litre engine.
GP1800 обладает невероятно плотным поворотом и стабильностью в более жестких условиях, а также максимальной скоростью 70 миль в час благодаря 1,8-литровому двигателю.
5. Yamaha WaveRunner FX SVHO
If you’re looking for a jet ski with comfort levels to match your superyacht then Yamaha’s three-seater FX SVHO is an ideal choice. Complete with all the expected luxury bells and whistles, including cruise control, a generous aft platform for easy boarding and an adjustable steering system, what really sets this model apart is the attention that has gone into its saddle. The two-piece design is tiered to allow all three passengers a brilliant view and finished in luxury materials with excellent lower back support for longer journeys. Speed freaks needn’t worry, however, Yamaha’s Super Vortex High Output 1812cc engine still packs a serious punch.
Если вы ищете водный мотоцикл с комфортными уровнями в соответствии с вашей суперяхтой, то трехместное FX SVHO Yamaha является идеальным выбором. В комплекте со всеми ожидаемыми роскошными колоколами и свистками, включая круиз-контроль, щедрую кормовую платформу для легкой посадки и регулируемую систему рулевого управления, то, что действительно отличает эту модель, - это внимание, которое ушло в седло. Двухкомпонентная конструкция имеет многоуровневое решение, позволяющее всем трем пассажирам получить великолепный вид и законченный в роскошных материалах с превосходной поддержкой нижней части спины для более длительных поездок. Speed ​​Freaks не нужно беспокоиться, однако, Yamaha Super Vortex High Output 1812cc двигатель все еще имеет серьезный удар.
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paolo210281-blog · 7 years
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Data Analysis: Mars Craters
1. The set of data selected is about Mars Craters. Presenta una base de datos global que incluye más de 300.000 cráteres de Marte 1 kilometro o más grandes que se han creado entre hace 4,2 y 3,8 mil millones de años durante un período de intenso bombardeo (es decir, impactos de asteroides, proto-planetas y cometas).
CRATER_ID: ID cráter para Sue interna, en la base a la región del planeta (), el “PASE” en las Que se identificó el cajón, ad El Orden En que se identificó1dieciséis1dieciséis
LATITUDE_CIRCLE_IMAGE: latitud del centro de la derivada de la ONU no lineales de Mínimos Cuadrados círculo fit un Seleccionados los vértices para identificar manualmente el Borde del cráter (hijo Las unidades Grados Decimales Norte)
LONGITUDE_CIRCLE_IMAGE: Longitud del centro de la derivada de la ONU no lineal de Mínimos Cuadrados círculo fit un Seleccionados los vértices para identificar manualmente el Borde del cráter (hijo Las unidades Grados Decimales Este)
DIAM_CIRCLE_IMAGE: Diámetro de la ONU no lineal de Mínimos Cuadrados círculo fit un Seleccionados los vértices para identificar manualmente el Borde del cráter (las unidades hijo km)
DEPTH_RIMFLOOR_TOPOG: Elevación medios de Cada Uno de los puntos manualmente Determinado N A lo largo (o Dentro de) el Borde del cráter (las unidades hijo km)
MORPHOLOGY_EJECTA_1: morfología eyecta Clasificado.
MORPHOLOGY_EJECTA_2: La morfología de la capa (s) en Si / Si Mismos. Este Sistema de Clasificación es Única párrafo Este trabajo.
MORPHOLOGY_EJECTA_3: textura y / o forma en general de la CAPA ALGUNAS de (s) / material de Expulsado hijo Que generalmente Único y merecen Clasificación morfológic
NUMBER_LAYERS: El Número Máximo de Capas cohesivas en any direction dirección acimutal Que podrian Ser identificados de forma fiable
2. The research question is that the relationship exists between depth, latitude, diameter, length with morphology.
La hipótesis nula (H0) nos podemos deducir en Cuenta Que No hay relacion Entre la Profundidad, latitud, diametro, Longitud con la morfologia
La hipótesis alternativa (H1) Podemos deducir que si existe relación entre la profundidad, latitud, diámetro, longitud con una morfología
3. “From the first spacecraft images returned of Mars, a new ejecta type was observed that was comprised of one or more cohesive layers of material. Throughout the literature, these have been referred to under a diverse range of names, including flower, composite, and various Types and Classes”
4. References:
4.1. Blasius, KR, Cutts, JA, 1980. Los patrones globales de cráter principal morfología de material expulsado en Marte en el Informe del Programa de Geología Planetaria 1980, la NASA Tech. Memorándum. 82385, pp. 147-149.
4.2.Horner, V.M., Greeley, R., 1987. Effects of elevation and ridged plains thicknesses on Martiancrater ejecta morphology. Proc. Lunar Planet. Sci. Conf, p. 2, XVII. J. Geophys. Res.92, B4, pp. E561-E569. doi: 10.1029/JB092iB04p0E561.
5. Statistically complete craters for diameters D! 1 km. This detailed database includes the location And size, morphology and morphometry of ejection, interior morphology and degradation state, and Whether the crater is a secondary impact. This database allowed exploring the type of global crater Distributions, depth and morphologies in an unprecedented detail that were used to reexamine
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wankelmuth · 6 months
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Hamburg, 2023
Photo: Roland Helbig
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