#eunis

[anitaho1981]

Eunis.com | 陳繹嵐 (陳嘉容) | Official Site | Beauty, Lifestyle, KOL

Eunis Chan shares her best collection of skincare and makeup products, etc, with all those who love beauty and care about wellness.

怎樣發揮面膜的最大效用？

一般面膜只會說明敷上面部的時間，而不會建議或說明應該什麼時候使用。如你有留意我早前有關晚霜的日誌，你會知道晚上是皮膚修復的黃金時間。 因此，保養型的面膜，如骨膠原及胎盤素的面膜等，就最適合在晚上最放鬆的黃金修護時間使用。清潔面膜，可以於洗澡後或作護理前使用。保濕面膜，可以在上妝前或潔面後使用，甚至乎是在長途機上或落機後馬上使用。妝前使用，是希望化妝時的粉底更貼面，而潔面後使用，意思是在塗抹化妝水之後使用，假如是乾燥肌可以多敷 5 分鐘，但盡可能不要超過 30 分鐘啊。

[sarasdesignblog]

EUNIS Dørup E-learning Award for Tomi Kauppinen, Yulia Guseva and Sara Gottschalk - Aalto Online Learning

We are very happy to announce that on June 11th, 2020 our paper Designing Digital Higher Education: Case Aalto Online Learning by Tomi Kauppinen, Yulia Guseva and Sara Gottschalk got the EUNIS Dørup E-learning Award 2020 in EUNIS 2020 Congress in its evening session Virtual Gala with live entertainment and presentation of EUNIS awards. EUNIS Dørup E-learning Award The EUNIS Dørup E-learning Award is given for the outstanding and innovative application of information technology (IT) in an educational setting. Read more...

-->> https://www.eunis.org/awards/dorup-award/

[mildredeu]

Apuesto todo a que esa persona,

la que sea más dueña de tus silencios que de tus palabras,

la querrás con una locura fuera de este mundo

y querrás habitar en ella en esta, la próxima, y hasta tu última vida.

[cassiscas]

Lady Satan reporting for duty #puggle #pugglesofinstagram #Eunis #LadySatanisanickname #calmdownTara #WNC

[grace-4ever]

My friend is going to the Midnight Premier of Star Wars.

(I live oversees, so it comes out tonight, okay?)

...I’m both anticipating and fearing tomorrow morning. Having no real interest in Star Wars, (It’s cool, but I just never got really into it,) I’ve made her give me a play-by-play.

No spoilers, but wish me luck. 

[the-telescope-times]

Strong evidence for coronal heating theory by nanoflares

Clear evidence now suggests that the heating mechanism depends on regular but intermittent explosive bursts of heat, rather than on continuous gradual heating.

NASA's EUNIS sounding rocket examined light from the sun in the area shown by the white line (imposed over an image of the sun from NASA's Solar Dynamics Observatory) then separated the light into various wavelengths (as shown in the lined images — spectra — on the right and left) to identify the temperature of material observed on the sun. The spectra provided evidence to explain why the sun's atmosphere is so much hotter than its surface.    Credit: NASA/EUNIS/SDO

Image credits: buffonescience7.wikispaces & http://folk.uio.no/gardini/sun.html

The Sun’s surface is blisteringly hot at 10,340° F (5,730° C) — but its atmosphere is another 300 times hotter. This has led to an enduring mystery for those who study the Sun: What heats the atmosphere to such extreme temperatures? Normally, when you move away from a hot source, the environment gets cooler, but some mechanism is clearly at work in the solar atmosphere, the corona, to bring the temperatures up so high. Clear evidence now suggests that the heating mechanism depends on regular but intermittent explosive bursts of heat, rather than on continuous gradual heating.

Read more at Astronomy Magazine.

More on our star here & here.

[thepopulation]

[newsvi]

NASA EUNIS Sees Evidence for Nanoflare Coronal Heating Scientists have recently gathered some of the strongest evidence to date to explain what makes the sun's outer atmosphere so much hotter than its surface. The new observations show temperatures in the atmosphere so hot that only one current theory explains them: something called nanoflares - a constant peppering of impulsive bursts of heating, none of which can be individually detected -- provide the mysterious extra heat. These new observations come from just six minutes worth of data from one of NASA's least expensive type of missions, a sounding rocket. The EUNIS mission, short for Extreme Ultraviolet Normal Incidence Spectrograph, launched on April 23, 2013, gathering a new snapshot of data every 1.3 seconds to track the properties of material over a wide range of temperatures in the complex solar atmosphere The unique capabilities of EUNIS enabled researchers to obtain these results. The spectrograph was able to clearly and unambiguously distinguish the observations representing the extremely hot material - emission lines showing light with a wavelength of 592.6 Angstrom, where an Angstrom is the size of an atom -- from a very nearby light wavelength of 592.2 Angstroms.