234th AAS Meeting, St. Louis MO

AAS 234

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Registration steps:

  1. Sign in if you're not already logged in. Then click "Register Myself."
  2. Select your registration option.
    • The registration rates are based on your current membership status; however, if you renew a lapsed membership and register for a meeting on the same day, you will be charged the nonmember registration rate. To register at the member rate, please wait until the following business day to register for the meeting and confirm you have been charged the correct fee before checking out.
    • Registration options for which you are ineligible are hidden.
    • Your eligibility will be reviewed if you select the student, emeritus, local educator, or amateur astronomer options.
    • If you select a one-day option, you will only be allowed in the meeting space on that day.
  3. Click "Save/Update Responses" before you select your program options and checkout.
  4. Add your program options and modify the quantity if needed.
  5. Use the "Update" and "Remove" buttons to change the quantity or remove an option.
  6. To register a guest, you must register yourself first and then click on the link "add a guest" under the heading My registration status.
6/9/2019 - 6/13/2019
St. Louis Union Station Hotel
1820 Market Street
St. Louis, MO 63103 United States

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Thursday, 06 June 2019

Your first abstract submission is included in your registration. Please select this option if you are submitting more than abstract. The cost is $45.00 for each addtional submission.
6/6/2019 - 6/6/2016

Saturday, 08 June 2019

6/8/2019 9:30 AM - 6/9/2019 3:00 PM
9:30 AM

Sunday, 09 June 2019

5:30 PM
7:00 PM - 8:30 PM
7:00 PM

Monday, 10 June 2019

The Interface Region Imaging Spectrograph (IRIS) observes the chromosphere and the transition region to understand how the solar atmosphere is energized. Since its launch in 2014 it has recorded more than 18,000 data sets in the Mg II h&k spectral range. Recovering the physical information from these data is crucial to answer how energy is transferred from the lower layers of the solar atmosphere to the hot corona. We will demonstrate a new technique that applies to the Mg II h&k spectra that quickly (in a few minutes) enables the recovery of the thermodynamic information within the atmosphere. This new approach is based on several machine learning and artificial intelligence methods. In this workshop we will discuss the concepts, estimated errors, and limitations of the method and, in a hands-on environment, how to implement and execute the code we have developed.
3:00 PM - 4:30 PM
3:00 PM

Wednesday, 12 June 2019

7:17 PM - 9:15 PM
7:17 PM

Thursday, 13 June 2019

This event is included in the FULL registration fee or One Day Only for Thursday
9:30 AM - 10:30 AM
9:30 AM