Or you can merge your branch back into the main version. When you are ready, you can commit changes to save your progress. You can create a copy of your source code, known as a branch, which you can then work on in parallel to the main version. Git stores your source code and its full development history locally in a repository. This strategy - using squash when merging - is often used when a Pull Request is closed.Git is a distributed, open-source version control system (VCS) that enables you to store code, track revision history, merge code changes, and revert to earlier code version when needed. It will appear as if the work for your feature had happened in just a single commit. In the end, this allows you to avoid the automatic commit that typically happens as a result of a merge. The effect is very similar to what we've discussed before: all changes will be combined just as with a normal merge - but by using the -squash option, instead of a merge commit being automatically created, you're left with local changes in your working copy which you can then commit yourself. Squashing is also an option when merging branches: $ git merge -squash feature/loginĪutomatic merge went well stopped before committing as requested In case you are using the Tower Git client, using Interactive Rebase to squash some commits is very simple: just select the commits you want to combine, right-click any of them, and select the "Squash Revisions." option from the contextual menu. If you mark one or more lines as "squash", they will be combined with the one above:Īfter entering a commit message for the new, combining commit, the Interactive Rebase is completed - and the three old commits have been squashed into one. Keep in mind that Interactive Rebase allows to perform many different actions on your commit history for our example case here, however, we are interested in the "squash" action keyword. We can do so by starting an Interactive Rebase session: $ git rebase -i HEAD~3Īn editor window will then open where you can choose how you want to manipulate the selected part of your commit history. But before doing so, you'd like to clean up and squash the new commits into a single one: Let's say you have completed your work on a new feature branch (in the below example "feature/login") and now want to merge it back into the "main" branch. ![]() Going deep into Interactive Rebase goes beyond the scope of this article (take a look at the First Aid Kit for Git for a series of free, short videos on this topic), but we'll walk through a simple example case together. You can manually squash your commits at any time using Git's "Interactive Rebase" feature. In this post, we'll talk about Interactive Rebase and Merge as the two main ways to squash commits. There are different ways and tools when it comes to squashing commits. There are pros and cons to both approaches, so it's mostly a matter of preference and convention. However, you cannot say that (a) or (b) is the "correct" way of doing things. This can be helpful in keeping things orderly! Some teams see a possible advantage in going with (a) and using squash: instead of many individual commits which might be unnecessary and potentially overwhelming, only a single commit appears in the main commit history.
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2020 YA YP4 will pass by at 1.5 and 2.1 million kilometres respectively.Įarlier on January 3, a gigantic 220-meter asteroid which was as tall as the Golden Gate Bridge is tall flew past the Earth at 6.9 million kilometres. Updated 4:48 AM ET, Wed November 24, 2021. This asteroid will be followed up by two more chunks of cosmic debris in the form of the 15-meter 2020 YA1 and the 21-meter 2020 YP4. A new simulation shows that when the DART mission hits the target asteroid, it could send it spinning and wobbling in a dramatic way.The dinosaurs didn’t have a space program, so when an asteroid headed toward Earth with their name on it 65 million years ago, they had no warning and no way to defend themselves. A NASA spacecraft that will deliberately crash into an asteroid has successfully launched. This asteroid will fly past the earth at a distance of 3.5 kilometres.Īnother 15-metre asteroid 2019 YB4 will fly by at a safe distance of 6.4 million kilometres. If it were to crash into the planet, the resulting impact would be the equivalent of 25 megatons to 50 megatons, the same as the largest nuclear bombs in existence today.Īccording to a statement by American space agency NASA, an asteroid called 2021 AC, which is twice the size of the Great Pyramid of Giza, is set to enter the Earth's orbit on Wednesday. The bigger asteroid, 2008 AF4, is nearly half a kilometre wide. This time, he had said the asteroid would fly past Earth sometime during early 2021. Notably, astrologer Nostradamus has made 6,338 predictions out of which 3797 prophecies have apparently proved correct. The report further said the smaller planets are expected to make a thinner impact. According to the Central for Near-Earth Object Studies (CNEOS), three of these are small, however, the other two asteroids approaching Earth are said to be bigger than the size of the Eiffel Tower. ![]() ![]() Five asteroids are approaching the Earth and are set to make a close approach today (January 6). Managed for NASA at the Jet Propulsion Laboratory, the Center for Near Earth Object Studies ( CNEOS) accurately characterizes the orbits of all known near-Earth objects, predicts their close approaches with Earth, and makes comprehensive impact hazard assessments in support of the agency’s. The prediction made by popular French astrologer Nostradamus has come true. Asteroid Watch: Keeping an Eye on Near-Earth Objects. ![]() Asteroids, bigger than Eiffel Tower to fly past Earth today A janitor I remember from Cleveland Elementary. Identifying Characteristic: Mexi-fro, pube-stache, pot-belly. ![]() He's also got a sort of round, cup-like face, and of course a huge gut, creating a resemblance to King Hippo of Mike Tyson's Punchout fame.īartolo Colon is nobody's favorite player. It's reminiscent of Andre the Giant, not well known for his good looks (but seemingly much more personable, and athletic for that matter). There's this horrible gericurl Mexi-fro that always sticks out from under his tiny cap like a neglected Chia pet.Īnd this pencil-thin grayish, pube-like "mustache" that he refuses to shave. His baseball-reference page is un-sponsored. Has been in the league for like 20 years and still doesn't speak English as far as I know. Nobody as far as I can tell, has ever been a fan of Bartolo Colon. Santana had more innings, strikeouts, complete games, shutouts, lower whip, lower ERA, scored with more chicks, cured more sick children and adopted more stray puppies than Bartolo that year, yet, well, we know how it turned out. I don’t want to look at a man’s mouth and see a vagina. Because it’s a problem if he’s growing it above his lip for fun. Pyoo'bstash An act involving the sexual union of one's face to a partner's unshaven and recently naired genitals, wherebye irrattic movement betwixt mouth and pubic area dislodges weakened hair follicles which then bind to one's face in the form of a mustache and/or beard. ![]() It doesn't help that this guy won a Cy Young Award that he blatantly didn't deserve, getting the nod over Johan Santana for the 2005 award, simply because he had 20 wins. Matt Damon pube stache at Green Zone New York premiere Matt’s little hairs Posted by Lainey on at 1:13 AM For a role It’s always for a role. ![]() How to resize an image for YouTube banner? ![]() Instead, you'll need to access your channel on a desktop computer and follow the instructions listed out in the previous question. Google and YouTube actually don't allow users to update their YouTube channel art via mobile. How to change a YouTube banner on iPhone? Click over to the Branding tab, then click Change to edit or add channel art. To change your YouTube banner, head over to your YouTube channel, then click the Customize Channel button. Check out all of the image sizes you need to keep in mind for different social media platforms. Your file size needs to be 6 MB or smaller, and we recommend a maximum width of 2560 pixels as an ideal YouTube banner size. Your safe area is only the middle 1546 x 423 pixels. 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Add in your brand name, your YouTube channel name, your vlogger pseudonym or perhaps the name of a new video series you want to promote. ![]() Your next step is to simply click on one of the text boxes and start typing to insert your own text. Create your YouTube channel art View more templates 2. ![]() The application of this type of force to low frequencies above the aurora was investigated by Li et al. This force is often referred to as the “Miller force” ( Miller, 1958). For example, averaging the force acting on an ion over the course of its gyration in a wave field with a spatial gradient yields a force oppositely directed to the spatial gradient in the wave amplitude. Ponderomotive forces are obtained by considering the net force by the electric and magnetic fields of an Alfvén wave acting on a particle over its gyration. Both of these mechanisms are nonresonant but can significantly accelerate ions as will be described in the following paragraphs. The second case deals with the case of scattering of ions by DAW, which are obliquely propagating with perpendicular wavelength comparable to the ion gyroradius. First, when the Alfvén waves have a perpendicular wavelength much larger than the ion gyroradius, a number of so-called “ponderomotive” forces can be exerted on the plasma that can lift charged particles to higher altitudes. There are multiple pathways through which Alfvén waves can exert influence on plasmas, but here we group them into two general categories. Low-frequency Alfvén waves, whose frequency is much less than the ion gyrofrequency, have also been argued to play an important role in the acceleration of plasma in the cusp and auroral regions. In Cross-Scale Coupling and Energy Transfer in the Magnetosphere-Ionosphere-Thermosphere System, 2022 1.4.1.3 Acceleration by interactions with low-frequency Alfvén waves We may thus proceed to use these data as a test of theories such as the KFR model, which treat the ATI process as scattering between the ground state and Volkov states in the continuum. In any case, the absence of sharp resonances in the 140 fsec electron spectra is very good evidence that bound states play a minimal role in ATI with circular polarization. This argument is explained in more detail in reference 14, and gives very similar results to the KFR calculations for circular polarization, as in reference 13. Evidently, transitions to continuum states is favored over transitions to these bound states, since even though high lying continuum states must have absorbed more photons and thus carry still more angular momentum, they can penetrate close to the ground state more easily because of their high energy. have their angular momentum L approaching their principal quantum number n. Essentially, these are high lying states that are relatively circular, i.e. ![]() ![]() A similar argument may be made for the bound states that come into resonance during ionization. There we found that the centrifugal barrier was an effective means of reducing the overlap, and hence the transition rate, between the ground state and continuum states of high angular momentum but low energy. Why have the resonances gone away? We speculate that the situation is essentially the same as for long pulses with circular polarization. The main difference is the absence of resonances in the circularly polarized case. The bottom trace in figure 3 the xenon ati spectrum for spectrum for 140 fsec 616 nm pulses with circular polarization. It now appears that at least one such system has been found: sub-picosecond photoionization of rare gases with circularly polarized light. We would like know if systems exist for which high order multiphoton ionization is truly nonresonant. The dominance of intermediate resonances complicates the business of calculating ATI. This fine structure has been associated with excited atomic states that are temporarily Stark shifted into resonance by the intense radiation. Reiss ( reference 13), integrated over the measured temporal and spatial profile of the laser pulse.Ħ16nm pulses, which reveal that each ATI peak really consists of a “fine structure” of electrons with different energies, ionized when the laser intensity was at different values. Bottom: A computer simulation of the experiment, using ionization rates from the Keldysh theory of H. 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