SOLARLAB
.docx
keyboard_arrow_up
School
Southwest University *
*We aren’t endorsed by this school
Course
110
Subject
Astronomy
Date
Jun 24, 2024
Type
docx
Pages
5
Uploaded by olivaselias20
Astronomy
Solar Lab
EPCC
Purpose
: Learn about the sun’s solar dynamics.
The Solar Basics:
Review these chapter links to learn more about our Sun: •
Astronomy (Chapter 15)
; Astronomy (Chapter 16)
Questions – Concisely answer within three (3) sentences:
1.
Sketch the interior of the sun and describe what each layer does.
S
2.
Describe how the sun’s hydrostatic equilibrium works in the sun.
The hydrostatic equilibrium of the Sun represents a finely tuned equilibrium wherein the gravitational force, drawing material inward towards the core, is offset by the outward pressure produced by nuclear fusion reactions within its core. This equilibrium plays a vital role in upholding the Sun's stable form and preventing its collapse due to gravitational forces.
Understanding NASA’s SDO mission. NOTE: DO NOT LOOK DIRECTLY AT THE SUN. We will use NASA data to analyze the sun’s surface features and dynamics. Go to the website to access this data: https://sdo.gsfc.nasa.gov/mission/
Plot Analysis (Refer to figure 1 and 2): In the menu bar, go to data, The sun now,
and select EVE
link.
Once you see a graph with data plotted on it, look for a Time and Date
section and input a start date 60 days prior to the current date. Input the current date for the end date, and select submit. Once 1
Astronomy
Solar Lab
EPCC
you get a new plot, save it as a PNG file. From this file, identify and highlight a day with the highest irradiance. Figure 2: Enter today's date and the date of 30 days prior (blue arrows), click “submit” (red Figure 1: Select "data', "EVE Data" highlighted in arrow), then save the data plot as a PNG file red, and access the irradiance data.
(black arrow)
Analyzing Solar Activity:
Go back to the main SDO website. Then go to main menu
→
select data→The
Sun Now. Of the array of images for today’s date, select the following and save them as a JPG file: 171 Å, 1600 Å, HMI Colorized Magnetogram, Intensitygram and HMI Dopplergram. Use the following link to learn what each data image describes about our Sun:
https://www.nasa.gov/missions/sdo/sun-science-stamps-highlight-a-decade-of-sun
watching-
from-space/
I n-situ solar image An image will be taken during class/lab of the Sun, which will be used to study the surface dynamics occurring on the Sun. Remember DO NOT LOOK DIRECTLY AT THE SUN
.
2
Astronomy
Solar Lab
EPCC
I mage and data submission In the table below, place those images and the plot you gathered from class and the website.
Image of Sun (class/lab)
•
171 Å (X- Ray)
•
1600 Å (UV)
•
HMI Colorized Magnetogram
• Intensitygram •
HMI Dopplergram
PNG Data Plot
Questions – Answer concisely within two (2) sentences. You may use your own sketches to help illustrate your answers : 3
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
- Access to all documents
- Unlimited textbook solutions
- 24/7 expert homework help