New User Special Price Expires in

Let's log you in.

Sign in with Facebook


Don't have a StudySoup account? Create one here!


Create a StudySoup account

Be part of our community, it's free to join!

Sign up with Facebook


Create your account
By creating an account you agree to StudySoup's terms and conditions and privacy policy

Already have a StudySoup account? Login here


by: Miss Jeanette Keebler


Miss Jeanette Keebler
GPA 3.74


Almost Ready


These notes were just uploaded, and will be ready to view shortly.

Purchase these notes here, or revisit this page.

Either way, we'll remind you when they're ready :)

Preview These Notes for FREE

Get a free preview of these Notes, just enter your email below.

Unlock Preview
Unlock Preview

Preview these materials now for free

Why put in your email? Get access to more of this material and other relevant free materials for your school

View Preview

About this Document

Class Notes
25 ?




Popular in Course

Popular in Earth And Space Sciences

This 18 page Class Notes was uploaded by Miss Jeanette Keebler on Wednesday September 9, 2015. The Class Notes belongs to ESS 590 at University of Washington taught by Staff in Fall. Since its upload, it has received 40 views. For similar materials see /class/192662/ess-590-university-of-washington in Earth And Space Sciences at University of Washington.

Similar to ESS 590 at UW

Popular in Earth And Space Sciences




Report this Material


What is Karma?


Karma is the currency of StudySoup.

You can buy or earn more Karma at anytime and redeem it for class notes, study guides, flashcards, and more!

Date Created: 09/09/15
Jupiter Aurora HST STIS WFPCZ PRC9804 ST SCI OPO January 7 1998 J Clarke University of Michigan and NASA L I 7 I1 5quot 3 I J 1 39 5 l Closure of cororation currents in the auroral zone Pulsating Xray spot 45 minute period a 39 c V v Relativistic electrons with a 1 q 40 minute intensity variations 2 o u on the dusk side high latitude Os i r pk Quasiperiodic explosive magnetic merging process E atquot i O w 33 o v 4391 3 r33 39 rquot 39339 Jo V um time n4 0 20 40 60 Brightness R Dun39ng quiet solar activity times Jupiter a stronger radio source than the Sun Aqu 115 251 if zumqu 15 2 zuuz J 31R 2e3qu 12m nun12 u 56 J JR p ux um um m 1 Emmy mm ed Y mm mm mm xmerchange events ow bursts C electrun bursts D upstream evems Processes controlling Jovian magnetosphere Jupiter magnetic field strength surface equatorial field 700000 nT Jupiter corotation rate 96 hours Internal plasma source 1 ton 51 lost from lo More than 100 known active volcanoes Torus made of 8 S 0 OH L If 3 I J 1 39 5 l Multiple Footprint Aurora Torus Alfven wing Vp W ma netic axis g 0 t be electflc current 39 I auroral zone MA 03 3 004 Ms gt 1 but fast Mach number lt 1 Io has equatorial aurora E vu Jupiter I XEu VP Sun ux tube ionospheric CLIFeM parallel trajecmry ionospheric current perpendicular Plasma Density and Flow lo s ionosphere is strongly advections dominated Plasma slowed in lo s ionosphere redirected around moon an then reaccelerated in the wake by 6RJ lonosphere has smaller density and smaller scale height on upstream side maximum density seen in the flanks 10x enhancement in wake 5x How is mass supplied to torus How is it heatedaccelerated IO SODIUM CLOUDS 15 R About 23 of iogenic material lost through Charge exchange Neutral Cloud Coid torus Neutral cloud Ne1000cm393 802 800 8 Na 8 TnTe1eV a M f a f C 39 N w I ll I Warm torus 90 of plasma Ne2000 Cm3 0 s n100ev Te5eV IO SODIUM CLOUDS 71 in lo frame Flow direction v 15 R Jet Electric fields associated with Jupiter s magnetospheric interaction with Io rip ions out of Io s collisionally thick atmosphere


Buy Material

Are you sure you want to buy this material for

25 Karma

Buy Material

BOOM! Enjoy Your Free Notes!

We've added these Notes to your profile, click here to view them now.


You're already Subscribed!

Looks like you've already subscribed to StudySoup, you won't need to purchase another subscription to get this material. To access this material simply click 'View Full Document'

Why people love StudySoup

Bentley McCaw University of Florida

"I was shooting for a perfect 4.0 GPA this semester. Having StudySoup as a study aid was critical to helping me achieve my goal...and I nailed it!"

Kyle Maynard Purdue

"When you're taking detailed notes and trying to help everyone else out in the class, it really helps you learn and understand the I made $280 on my first study guide!"

Steve Martinelli UC Los Angeles

"There's no way I would have passed my Organic Chemistry class this semester without the notes and study guides I got from StudySoup."


"Their 'Elite Notetakers' are making over $1,200/month in sales by creating high quality content that helps their classmates in a time of need."

Become an Elite Notetaker and start selling your notes online!

Refund Policy


All subscriptions to StudySoup are paid in full at the time of subscribing. To change your credit card information or to cancel your subscription, go to "Edit Settings". All credit card information will be available there. If you should decide to cancel your subscription, it will continue to be valid until the next payment period, as all payments for the current period were made in advance. For special circumstances, please email


StudySoup has more than 1 million course-specific study resources to help students study smarter. If you’re having trouble finding what you’re looking for, our customer support team can help you find what you need! Feel free to contact them here:

Recurring Subscriptions: If you have canceled your recurring subscription on the day of renewal and have not downloaded any documents, you may request a refund by submitting an email to

Satisfaction Guarantee: If you’re not satisfied with your subscription, you can contact us for further help. Contact must be made within 3 business days of your subscription purchase and your refund request will be subject for review.

Please Note: Refunds can never be provided more than 30 days after the initial purchase date regardless of your activity on the site.