TY - JOUR
T1 - Stellar Activity and Parker Solar Probe
T2 - American Astronomical Society Meeting
AU - Korreck, K. E.
AU - Szabo, A.
AU - Nieves Chinchilla, T.
AU - Alzate, N.
AU - Wallace, S.
AU - Niembro, T.
AU - Lavraud, B.
AU - Stevens, M. L.
AU - Whittlesey, P.
AU - Livi, R.
AU - Kasper, J.
AU - Luhman, J.
AU - Bale, S.
AU - Paulson, K.
AU - Higginson, A.
AU - Case, T.
AU - Rouillard, A.
AU - Koulouvamkos, A.
AU - Poirier, N.
AU - Pulupa, M.
AU - Goetz, K.
AU - Larson, D.
AU - Malaspina, D.
AU - Morgan, H.
AU - Narock, A.
AU - Schwadron, N.
AU - Bonnell, J.
AU - Harvey, P.
AU - Wygant, J.
N1 - Conference code: 235
PY - 2020/1/1
Y1 - 2020/1/1
N2 - In Parker Solar Probe's (PSP) first orbit, in situ thermal plasma
measurements were made between 35 and 55 solar radii from the Sun, an
environment that has not been previously explored, with the SWEAP
instrument suite. During the first orbit of PSP, the spacecraft flew
through two coronal mass ejections (CMEs) one on October 31, 2018 as it
entered an encounter and the second CME on November 11, 2018 as it
exited encounter. This CME on November 11 was directed away from the
Earth and was not visible from Earth based telescopes due to this
configuration. However, Parker Solar Probe and the STEREO A spacecraft
were able to make observations of this CME. This paper looks at the
source, propagation and implications to space weather of the closest in
situ measured Coronal Mass Ejection to the Sun. In addition, a
discussion of the implications for stellar activity as well as the
general radiation environment surrounding a star.
AB - In Parker Solar Probe's (PSP) first orbit, in situ thermal plasma
measurements were made between 35 and 55 solar radii from the Sun, an
environment that has not been previously explored, with the SWEAP
instrument suite. During the first orbit of PSP, the spacecraft flew
through two coronal mass ejections (CMEs) one on October 31, 2018 as it
entered an encounter and the second CME on November 11, 2018 as it
exited encounter. This CME on November 11 was directed away from the
Earth and was not visible from Earth based telescopes due to this
configuration. However, Parker Solar Probe and the STEREO A spacecraft
were able to make observations of this CME. This paper looks at the
source, propagation and implications to space weather of the closest in
situ measured Coronal Mass Ejection to the Sun. In addition, a
discussion of the implications for stellar activity as well as the
general radiation environment surrounding a star.
M3 - Meeting Abstract
SN - 0002-7537
VL - 52
SP - 125
JO - Bulletin of the American Astronomical Society
JF - Bulletin of the American Astronomical Society
IS - 1
Y2 - 4 January 2020 through 8 January 2020
ER -