Search for: All records

Creators/Authors contains: "Kamenetzky, Julia"

« Prev Next »

Total Resources

2

Resource Type
Conference Paper

0

Conference Proceeding

0

Dataset

0

Journal Article

2

Workshop Report

0

Availability
Full Text / Resource Available

2

Citation Only

0

Save Results
Excel (limit 2000)
CSV (limit 5000)
XML (limit 5000)

Have feedback or suggestions for a way to improve these results?
!

Note: When clicking on a Digital Object Identifier (DOI) number, you will be taken to an external site maintained by the publisher. Some full text articles may not yet be available without a charge during the embargo (administrative interval).
What is a DOI Number?

Some links on this page may take you to non-federal websites. Their policies may differ from this site.

New Insights into the Physical Conditions and Internal Structure of a Candidate Proto-globular Cluster

https://doi.org/10.3847/1538-4357/ab0d1e

Finn, Molly K. ; Johnson, Kelsey E. ; Brogan, Crystal L. ; Wilson, Christine D. ; Indebetouw, Remy ; Harris, William E. ; Kamenetzky, Julia ; Bemis, Ashley ( April 2019 , The Astrophysical Journal)

Full Text Available
Acceleration of Coronal Mass Ejection Plasma in the Low Corona as Measured by the Citizen CATE Experiment

https://doi.org/10.1088/1538-3873/ab558c

Penn, Matthew J. ; Baer, Robert ; Walter, Donald ; Pierce, Michael ; Gelderman, Richard ; Ursache, Andrei ; Elmore, David ; Mitchell, Adrianna ; Kovac, Sarah ; Hare, Honor ; et al ( December 2019 , Publications of the Astronomical Society of the Pacific)

Abstract
The citizen Continental-America Telescopic Eclipse (CATE) Experiment was a new type of citizen science experiment designed to capture a time sequence of white-light coronal observations during totality from 17:16 to 18:48 UT on 2017 August 21. Using identical instruments the CATE group imaged the inner corona from 1 to 2.1 RSun with 1.″43 pixels at a cadence of 2.1 s. A slow coronal mass ejection (CME) started on the SW limb of the Sun before the total eclipse began. An analysis of CATE data from 17:22 to 17:39 UT maps the spatial distribution of coronal flow velocities from about 1.2 to 2.1 RSun, and shows the CME material accelerates from about 0 to 200 km s⁻¹across this part of the corona. This CME is observed by LASCO C2 at 3.1–13 RSun with a constant speed of 254 km s⁻¹. The CATE and LASCO observations are not fit by either constant acceleration nor spatially uniform velocity change, and so the CME acceleration mechanism must produce variable acceleration in this region of the corona.

more » « less