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On August 21, 2017, a total eclipse of the Sun will be visible across the entire contiguous United States. It will trace out a band, approximately 70 miles wide across fourteen states, being first visible shortly after 10:15am PDT at Oregon's Pacific coast, and finally finishing in Charleston, South Carolina. The longest duration of totality will be 2 minutes and 42 seconds, which will occur in Giant City State Park, near Carbondale, Illinois. A partial eclipse will be visible across a much broader band including all of North America, northern South America, Western Europe, and even parts of Africa. To see an interactive map of the path of the eclipse, please visit Loud Look Ladies Pixie Rouched Flat Pull On Flat Slouch Ankle Boots Size 38 Black j4bnytXJQJ
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On August 11, 2017, we started an MHD computation of the solar corona, in preparation for our prediction of what the solar corona will look like during this eclipse. We used data measured by the HMI magnetograph aboard NASA's Haflinger Womens AR Jack Flat Black u3JIge0bW
. We used a combination of HMI synoptic maps, including data for Carrington rotation 2192 combined with data from a part of Carrington rotation 2193 measured up to 12:00 UTC on August 11, 2017. You can read the details about the evolution of the photospheric magnetic field that was used to make our prediction.

This final prediction of the state of the solar corona during the eclipse was posted on August 16, 2017. This updates the preliminary prediction posted on July 31, 2017 with newer magnetic field data.

Our prediction is based on a magnetohydrodynamic model of the solar corona with improved energy transport. While our earlier predictions incorporated a more simplistic heating formalism, for the first time, here, we have applied a wave-turbulence-driven (WTD) methodology to heat the corona. This model better reproduces the underlying physical processes in the corona, and has the potential to produce a more accurate eclipse prediction. Additionally, these simulations are among the largest we have performed, using 65 million grid points. For technical details about our model, please see the publications .

For our final prediction, we introduced magnetic shear along polarity inversion lines (PILs - lines separating positive and negative polarity regions) where filament channels were observed in EUV emission by SDO/AIA. This is a well-known feature of large-scale coronal magnetic fields that we have not accounted for in past predictions. The handedness of the shear is deduced from the combination of a magnetofrictional model and a surface flux transport model; special thanks go to Duncan Mackay (University of St. Andrews), Anthony Yeates (Durham University), and Lisa Upton (High Altitude Observatory) for their help - see Carolbar Womens Contraststitching Sexy High Heel Over The Knee Boots Black S2wijTx1UD
. The introduction of shear qualitatively changes the shape of the streamers and the connectivity of the underlying fields, and increases the free magnetic energy in the corona. It can even produce a CME .

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The University of New Mexico

Friday, October 19, 2018 6:00 PM Reception 7:00 PM Dinner Awards Ceremony UNM Student Union Ballrooms

Registration Sponsorship Opportunities available soon.

Proceeds from the Distinguished Achievement Awards Dinner help fund the Law Alumni Association's programming and full-tuition merit scholarships at the Law School.

The Law Alumni/ae Association has been counseled to not honor judges currently presiding on the bench due to the awards ceremony being a fundraiser.

Watch the 2017 honorees' tribute video

Watch Now

Distinguished Achievement Award Criteria

Awarded to an alumnus/a, faculty member or member of the legal community who fits the following criteria:

NEW! Alumni Promise Award Criteria

Awarded to an alumnus/a whose service to the UNM School of Law community embodies the UNMSOL Alumni Association’s vision of Honoring the Past | Building the Future, and who:

The Alumni Merit Scholarship was extremely important to me. It was a factor in my decision to stay in New Mexico, attend law school here, and become a New Mexico lawyer. As a recipient of the scholarship, I realized that I had the support of the entire legal community of New Mexico, and it motivated me to work even harder in law school. The Scholarship afforded me so many important opportunities, and I am thrilled to be able to give back to New Mexico and the UNM School of Law as an alumna.

The Law Alumni/ae Association full-tuition scholarship is life changing in so many ways. For me I think it is particularly humbling and motivating to know that there are people out there who support my goals, so much so that they are willing to finance my legal education. This scholarship removes a significant burden off of me as a student and allows me to focus my time and energy on becoming the best lawyer I can be. The confidence this scholarship inspires is truly incredible and I could not be more grateful for the support.

When I applied to law school, I never thought that I would get in, let alone receive a scholarship. Besides giving me and my family the financial support I needed to be able to attend law school, the Scholarship gave me the important message that I was "law school material," and really deserved to be here. Attending UNM School of Law has changed my life and given me amazing opportunities, and I'm really excited about the directions my career path is already taking. Words are inadequate to describe the feeling of gratitude I have that the Alumni Board decided to take a chance on me, and gave me the opportunity to become a part of this community.

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Grapeseed Oil - contains linoleic acid which has been proven in treating acne, eczema and other dermatitis. The oil is useful in moisturizing the skin, promoting hair growth and helping to repair damaged skin cells.

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