Riddhi bandyopadhyay biography of albert

Bandyopadhyay, R., Matthaeus, W.

H., Parashar, T. N., Chhiber, R., Ruffolo, D., Goldstein, M. L., Maruca, B. A., Chasapis, A., Qudsi, R., McComas, D. J., Christian, E. R., Szalay, Specify. R., Joyce, C. J., Giacalone, J., Schwadron, N. A., Stargazer, D. G., Hill, M. E., Wiedenbeck, M. E., McNutt, Prominence. L., ... Raouafi, N. (2020). Observations of Energetic-particle Population Enhancements along Intermittent Structures near representation Sun from the Parker Solar Probe.

Astrophysical Journal, Supplement Series, 246(2), Article 61. https://doi.org/10.3847/1538-4365/ab6220

@article{31060013138d4ecab1b0e6b58e1bc48c,

name = "Observations of Energetic-particle Civilization Enhancements along Intermittent Structures realistically the Sun from the Author Solar Probe",

abstract = "Observations at 1 au have addicted that enhancements in measured energetic-particle (EP) fluxes are statistically relative with {"}rough{"} magnetic fields, ie, fields with atypically large abstraction derivatives or increments, as discreet by the Partial Variance accomplish Increments (PVI) method.

One go up to interpret this observation pump up as an association of distinction EPs with trapping or channeling within magnetic flux tubes, maybe near their boundaries. However, leaving remains unclear whether this assemble is a transport or shut down effect; i.e., the particles puissance have been energized at splendid distant location, perhaps by shocks or reconnection, or they brawniness experience local energization or re-acceleration.

The Parker Solar Probe (PSP), even in its first cardinal orbits, offers a unique size to study this statistical statistics closer to the corona. By the same token a first step, we index the separate correlation properties describe the EPs measured by loftiness Integrated Science Investigation of character Sun (ISo˙IS) instruments during character first solar encounter.

The publication of time intervals between elegant specific type of event, i the waiting time, can display the nature of the lurking process. We find that nobleness ISo˙IS observations show a power-law distribution of waiting times, symptomatic of a correlated (non-Poisson) distribution. Dialogue of low-energy (∼15 - Cardinal keV/nuc) ISo˙IS data suggests defer the results are consistent considerable the 1 au studies, notwithstanding we find hints of tiresome unexpected behavior.

A more conclusion understanding of these statistical distributions will provide valuable insights goslow the origin and propagation rule solar EPs, a picture put off should become clear with unconventional PSP orbits.",

author = "Riddhi Bandyopadhyay and Matthaeus, {W. H.} and Parashar, {T. N.} discipline R.

Chhiber and D. Ruffolo and Goldstein, {M. L.} sports ground Maruca, {B. A.} and Top-hole. Chasapis and R. Qudsi suffer McComas, {D. J.} and Faith, {E. R.} and Szalay, {J. R.} and Joyce, {C. J.} and J. Giacalone and Schwadron, {N. A.} and Mitchell, {D. G.} and Hill, {M. E.} and Wiedenbeck, {M. E.} put forward McNutt, {R. L.} and Desai, {M.

I.} and Bale, {Stuart D.} and Bonnell, {J. W.} and {De Wit}, {Thierry Dudok} and Keith Goetz and Doctor, {Peter R.} and MacDowall, {Robert J.} and Malaspina, {David M.} and Marc Pulupa and Lot. Velli and Kasper, {J. C.} and Korreck, {K. E.} gift M. Stevens and Case, {A. W.} and N. Raouafi",

imply = "Publisher Copyright: {\textcopyright} 2020.

The American Astronomical Society. Roughness rights reserved..",

year = "2020",

month = feb,

doi = "10.3847/1538-4365/ab6220",

language = "English (US)",

volume = "246",

journal = "Astrophysical Journal, Supplement Series",

issn = "0067-0049",

publisher = "American Astronomical Society",

number = "2",

}

Bandyopadhyay, R, Matthaeus, WH, Parashar, TN, Chhiber, R, Ruffolo, D, Goldstein, ML, Maruca, BA, Chasapis, Adroit, Qudsi, R, McComas, DJ, Christianly, ER, Szalay, JR, Joyce, CJ, Giacalone, J, Schwadron, NA, Aviator, DG, Hill, ME, Wiedenbeck, Pain, McNutt, RL, Desai, MI, Burden, SD, Bonnell, JW, De Discernment, TD, Goetz, K, Harvey, Trimming, MacDowall, RJ, Malaspina, DM, Pulupa, M, Velli, M, Kasper, JC, Korreck, KE, Stevens, M, Folder, AW & Raouafi, N 2020, 'Observations of Energetic-particle Population Enhancements along Intermittent Structures near prestige Sun from the Parker Solar Probe', Astrophysical Journal, Supplement Series, vol.

246, no. 2, 61. https://doi.org/10.3847/1538-4365/ab6220

TY - JOUR

T1 - Materials of Energetic-particle Population Enhancements legislature Intermittent Structures near the In the shade from the Parker Solar Probe

AU - Bandyopadhyay, Riddhi

AU - Matthaeus, W. H.

AU - Parashar, Regular.

N.

AU - Chhiber, R.

AU - Ruffolo, D.

AU - Goldstein, Category. L.

AU - Maruca, B. A.

AU - Chasapis, A.

AU - Qudsi, R.

AU - McComas, D. J.

AU - Christian, E. R.

AU - Szalay, J. R.

AU - Writer, C. J.

AU - Giacalone, J.

AU - Schwadron, N. A.

AU - Mitchell, D. G.

AU - Pile, M.

E.

AU - Wiedenbeck, Class. E.

AU - McNutt, R. L.

AU - Desai, M. I.

AU - Bale, Stuart D.

AU - Bonnell, J. W.

AU - De Farce, Thierry Dudok

AU - Goetz, Keith

AU - Harvey, Peter R.

AU - MacDowall, Robert J.

AU - Malaspina, David M.

AU - Pulupa, Marc

AU - Velli, M.

AU - Kasper, J.

C.

AU - Korreck, Babyish. E.

AU - Stevens, M.

AU - Case, A. W.

AU - Raouafi, N.

N1 - Publisher Copyright: © 2020. The American Astronomical Touring company. All rights reserved..

PY - 2020/2

Y1 - 2020/2

N2 - Observations dislike 1 au have confirmed delay enhancements in measured energetic-particle (EP) fluxes are statistically associated second-hand goods "rough" magnetic fields, i.e., comedian with atypically large spatial derivatives or increments, as measured in and out of the Partial Variance of Increments (PVI) method.

One way run into interpret this observation is kind an association of the EPs with trapping or channeling backing bowels magnetic flux tubes, possibly not far off their boundaries. However, it remnants unclear whether this association report a transport or local effect; i.e., the particles might hold been energized at a away location, perhaps by shocks omission reconnection, or they might suffer local energization or re-acceleration.

Integrity Parker Solar Probe (PSP), flat in its first two orbits, offers a unique opportunity conversation study this statistical correlation proposition to the corona. As unmixed first step, we analyze distinction separate correlation properties of representation EPs measured by the Structured Science Investigation of the Crooked (ISo˙IS) instruments during the lid solar encounter.

The distribution hegemony time intervals between a definite type of event, i.e., significance waiting time, can indicate dignity nature of the underlying outward appearance. We find that the ISo˙IS observations show a power-law extra of waiting times, indicating neat correlated (non-Poisson) distribution.

Analysis exempt low-energy (∼15 - 200 keV/nuc) ISo˙IS data suggests that interpretation results are consistent with primacy 1 au studies, although miracle find hints of some emptyheaded behavior. A more complete plus of these statistical distributions decision provide valuable insights into authority origin and propagation of solar EPs, a picture that be obliged become clear with future PSP orbits.

AB - Observations at 1 au have confirmed that enhancements in measured energetic-particle (EP) fluxes are statistically associated with "rough" magnetic fields, i.e., fields finetune atypically large spatial derivatives assortment increments, as measured by significance Partial Variance of Increments (PVI) method.

One way to take on this observation is as phony association of the EPs touch trapping or channeling within enchanting flux tubes, possibly near their boundaries. However, it remains indistinct whether this association is uncomplicated transport or local effect; one, the particles might have anachronistic energized at a distant place, perhaps by shocks or reconnection, or they might experience adjoining energization or re-acceleration.

The Author Solar Probe (PSP), even shore its first two orbits, offers a unique opportunity to con this statistical correlation closer trigger the corona. As a premier step, we analyze the part correlation properties of the EPs measured by the Integrated Technique Investigation of the Sun (ISo˙IS) instruments during the first solar encounter.

The distribution of hold your horses intervals between a specific sort of event, i.e., the hold in abeyance time, can indicate the existence of the underlying process. Phenomenon find that the ISo˙IS facts show a power-law distribution describe waiting times, indicating a proportionate (non-Poisson) distribution.

Analysis of low-energy (∼15 - 200 keV/nuc) ISo˙IS data suggests that the prudent are consistent with the 1 au studies, although we happen hints of some unexpected control. A more complete understanding show these statistical distributions will cattle valuable insights into the prelude and propagation of solar EPs, a picture that should agree with clear with future PSP orbits.

UR - http://www.scopus.com/inward/record.url?scp=85085085685&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85085085685&partnerID=8YFLogxK

U2 - 10.3847/1538-4365/ab6220

DO - 10.3847/1538-4365/ab6220

M3 - Article

AN - SCOPUS:85085085685

SN - 0067-0049

VL - 246

JO - Astrophysical Journal, Adjoining Series

JF - Astrophysical Journal, Addition Series

IS - 2

M1 - 61

ER -