Clumpy

If you want to have a quick overview whether CLUMPY serves for your purposes, have a look at the Introduction and browse the clumpy executable: options and plots section or the Picture gallery. If you have decided to use CLUMPY, download it from the GitLab repository and consult the Download and Installation section. Start using it from our Quick start tutorial and learn more about of the various modules of CLUMPY in the Physics and equations section. An automatically generated PDF version of this documentation can be retrieved here.

One surprising revelation from the map is that matter isn't as "clumpy" as our current best model of the universe suggests it should be, meaning something could be missing from our standard cosmological model.

clumpy

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I have made this twice now. I added two whisked egg whites to the wet mixture to make the granola more clumpy and crunchy! The second round I made with dried montmorency cherries and apricots. Very good!

This is a \u201Chands-on\u201D project, meaning that you will need to get your hands into it. Of course, they should be scrupulously clean, which is easy nowadays\u2026now that we all have hand sanitizer with us at all times. If you like your granola clumpy, when you distribute it onto the baking sheet, squeeze small handfuls of it into clumps, then drop them on the baking sheet.

Further studies of clumpy galaxies confirm that they are very young galaxies with lots of star formation occuring in the massive clumps, which may be embedded within a slightly older, smoother distribution of stars. Their prevalence means they are likely to be an early phase in the development of most, if not all, galaxies.

As I mentioned in my previous post, for Galaxy Zoo: Hubble we added a series of questions in order to find out about the appearance of clumpy galaxies. This will provide us with a catalogue of their properties that is larger and more consistent than any before. By analysing this data we hope to learn much more about these galaxies. For example, there appears to be a rough developmental sequence from asymmetric clumpy galaxies, to symmetric clumpy galaxies, to clumpy galaxies dominated by a bright, central clump, and finally to spiral galaxies. Other clumpy galaxies may merge together to form ellipticals. By comparing the numbers and properties of these different types of galaxies we will be able to confirm or refute this picture, and better understand the origins of the galaxy population.

The history of the transition from a neutral intergalactic medium (IGM) to one that is almost fully ionized can reveal the character of cosmological ionizing sources. We study the evolution of the volume filling factors of H II and He III regions in a clumpy IGM and discuss the implications for rival reionization scenarios of the rapid decline observed at z>3 in the space density of optical and radio-loud quasars and of the large population of star-forming galaxies recently discovered at the same epoch. The hydrogen component in a highly inhomogeneous universe is completely reionized when the number of photons emitted above 1 ryd in one recombination time equals the mean number of hydrogen atoms. If stellar sources are responsible for keeping the IGM ionized at z=5, the rate of star formation at this epoch must be comparable or greater than the one inferred from optical observations of galaxies at z3 and the mean metallicity per baryon in the universe >0.002 solar. An early generation of stars in dark matter halos with circular velocities, vcirc50 km s-1, possibly one of the main sources of UV photons at high z, could be detectable with the Next Generation Space Telescope. Models in which the quasar emissivity declines rapidly at z>3 predict a late He II reionization epoch, a feature that could explain the recent detection of patchy He II Lyα at z=2.9 by Reimers et al. and the abrupt change observed by Songaila at about the same epoch of the Si IV /C IV ratio, but appear unable to provide the required number of hydrogen-ionizing photons at z5.

NEWS: major culinary breakthrough has been achieved. I've made clumpy, cluster-y granola without adding a bajillion sticks of butter or raw eggs or the like. The feeling of accomplishment and discovery I have at this moment is quite high, and I'd like to pass it on.

Now, onto the question of clumps. I'm happy to eat granola that is less clumpy and more cereal-like in texture, but clumpy granola is ideal. It's easier to eat on the go with your fingers (perfect hiking food), and it has a more satisfying crunch.

Across the board, marketers see far stronger results when they use RFMC data versus only using RFM. By focusing on clumpy consumers as their most valuable customers, brands can realize far stronger CLV and profitability.

A variety of different factors can drive clumpy behavior. In the case of content, the key driver is availability. For example, Netflix releases a new season of a given show, and suddenly everyone wants to watch it ASAP. They literally plan their lives around it.

As a part of our research, we examined multiple retailers in specific product categories. Among the key findings were that millennials are more clumpy than other generations and that women are clumpier than men.

By understanding clumpy behavior, knowing to look for it and analyzing the level of clumpiness, marketers and other key decision makers gain a new metric for measuring and predicting CLV and choosing which customers to focus on and when. They can also gain a better understanding of customer satisfaction and react to it faster.

Infections may cause vaginal discharge to appear thick, white, and clumpy. A vaginal yeast infection, for instance, produces this consistency of discharge. If a yeast infection is present, a person may experience accompanying symptoms, such as:

We are LOVING this granola in our household! I just made your rhubarb almond flour muffins and it got me to wondering if I could use the roasted almond oil from that recipe in the extra clumpy granola recipe?

We often receive questions about why matcha has clumps. There is a misconception that clumpy matcha equates to "bad" matcha, which is far from the truth. Keep reading on why clumps are an indicator of high quality, stone-ground matcha and for a tip on how to ensure each cup is clump-free.

Then, the mixture was too dry, so I upped the amount of the liquid ingredients to match my go-to granola recipe, and it turned out mega clumpy, with an irresistible, sweet and wholesome crunch. You can see the texture best in the photo below, which I snapped after I quit tinkering.

Once again I start with darks and build up lighter layers until we get a sense of that clumpy woollen coat. Occasionally I change settings like opacity and dab spacing as required, but all in all I like the way it handles.

Using too many strokes of mascara leads to droopy, product-laden lashes. So, here are some tips on how to fix clumpy lashes that can ruin your whole look on an important day. Sometimes, a hurried application may lead to an uneven look, and some of the chunks freeze on a few lashes, making them look downright ugly, for lack of a better word.

Old, unused mascara will give you the caked up clumpy look and eventually can also lead to eye irritation. So, one great tip for having the perfect lashes is to use your mascara while it is still new. Buy a long lasting mascara that is waterproof and smudge-free. Also, find a mascara that has a mascara applicator which has plenty of space in between the bristles. A bristle like that goes in between each and every lash, covering each one, for a fuller, natural look. Too many plush bristles on a mascara applicator will give you the clumped look when you apply it over your lashes.

When it comes to makeup, there is nothing unfixable. So, why endure the discomfort that clumpy lashes give you? Not only do they come in between your vision but also they spoil your look. So, now that you know how to fix clumpy lashes, what is holding you back? Learn from the tips and tricks mentioned above and get started. Your makeup should define your features and enhance your look. So, do not let any makeup products ruin your day. Also, applying the mascara gently with precision is the key.

This is the most common reason why pre workouts turn clumpy or hard. As the powdered ingredients are hygroscopic, they naturally begin to attract moisture from the air and container at room temperature.

The quickest, safest and most effective way to deal with a clumpy pre-workout is to empty your clumpy pre-workout into a blender, and blitz until it's turned back into a fine powder. Some blenders now even come with special attachments that are specifically for making powders so if you have one of those, whack it on, if not, the normal attachment should do the job. Remember, always remove the silica packet before doing this.

The key takeaway from this complete guide is that most of the time (excluding the three points mentioned previously) clumpy pre-workout doesn't mean that there is anything wrong with your powder and it can be easily fixed with a quick blitz in the blender without impacting its effectiveness.

Firstly always keep the silica gel packet buried in your pre-workout container. This is the most common reason why pre-workouts turn clumpy or hard. As the powdered ingredients are hygroscopic, they naturally begin to attract moisture from the air and container at room temperature. Silica gel packets prevent the powder from attracting moisture.

RIKEN astrophysicists have found strong evidence that the clumpy structure of the 450-year-old remnant of a supernova explosion originated from the explosion itself and not from processes that occurred after the explosion1. This goes some way towards unveiling the mystery that shrouds supernova explosions.

X-ray images of the remnant reveal that it has a distinctly clumpy appearance, and much speculation exists about the origin of this clumpiness. There are two main theories: one posits that the clumps were present in the explosion itself, whereas the other hypothesizes that they arose during the subsequent dispersion of gas. 2ff7e9595c