@article{Chhiber2021,
	title = {Magnetic field line random walk and solar energetic particle path lengths {Stochastic} theory and {PSP}/{IS} circle dot {IS} observations},
	volume = {650},
	issn = {0004-6361},
	url = {https://doi.org/10.1051/0004-6361/202039816},
	doi = {10.1051/0004-6361/202039816},
	abstract = {Context. In 2020 May-June, six solar energetic ion events were observed by the Parker Solar Probe/IS circle dot IS instrument suite at approximate to 0.35 AU from the Sun. From standard velocity-dispersion analysis, the apparent ion path length is approximate to 0.625 AU at the onset of each event.},
	journal = {Astronomy \& Astrophysics},
	author = {Chhiber, R. and Matthaeus, W. H. and Cohen, C. M. S. and Ruffolo, D. and Sonsrettee, W. and Tooprakai, P. and Seripienlert, A. and Chuychai, P. and V Usmanov, A. and Goldstein, M. L. and McComas, D. J. and Leske, R. A. and Szalay, J. R. and Joyce, C. J. and Cummings, A. C. and Roelof, E. C. and Christian, E. R. and Mewaldt, R. A. and Labrador, A. W. and Giacalone, J. and Schwadron, N. A. and Mitchell, D. G. and Hill, M. E. and Wiedenbeck, M. E. and Jr. McNutt, R. L. and I Desai, M.},
	year = {2021},
	note = {Publisher: Edp Sciences S A
Type: Article
tex.date-modified: 2022-04-12 11:34:55 +0100},
}

{"_id":"RjHogMEB5Re9cLSuz","bibbaseid":"chhiber-matthaeus-cohen-ruffolo-sonsrettee-tooprakai-seripienlert-chuychai-etal-magneticfieldlinerandomwalkandsolarenergeticparticlepathlengthsstochastictheoryandpspiscircledotisobservations-2021","author_short":["Chhiber, R.","Matthaeus, W. H.","Cohen, C. M. S.","Ruffolo, D.","Sonsrettee, W.","Tooprakai, P.","Seripienlert, A.","Chuychai, P.","V Usmanov, A.","Goldstein, M. L.","McComas, D. J.","Leske, R. A.","Szalay, J. R.","Joyce, C. J.","Cummings, A. C.","Roelof, E. C.","Christian, E. R.","Mewaldt, R. A.","Labrador, A. W.","Giacalone, J.","Schwadron, N. A.","Mitchell, D. G.","Hill, M. E.","Wiedenbeck, M. E.","Jr. McNutt, R. L.","I Desai, M."],"bibdata":{"bibtype":"article","type":"article","title":"Magnetic field line random walk and solar energetic particle path lengths Stochastic theory and PSP/IS circle dot IS observations","volume":"650","issn":"0004-6361","url":"https://doi.org/10.1051/0004-6361/202039816","doi":"10.1051/0004-6361/202039816","abstract":"Context. In 2020 May-June, six solar energetic ion events were observed by the Parker Solar Probe/IS circle dot IS instrument suite at approximate to 0.35 AU from the Sun. From standard velocity-dispersion analysis, the apparent ion path length is approximate to 0.625 AU at the onset of each event.","journal":"Astronomy & Astrophysics","author":[{"propositions":[],"lastnames":["Chhiber"],"firstnames":["R."],"suffixes":[]},{"propositions":[],"lastnames":["Matthaeus"],"firstnames":["W.","H."],"suffixes":[]},{"propositions":[],"lastnames":["Cohen"],"firstnames":["C.","M.","S."],"suffixes":[]},{"propositions":[],"lastnames":["Ruffolo"],"firstnames":["D."],"suffixes":[]},{"propositions":[],"lastnames":["Sonsrettee"],"firstnames":["W."],"suffixes":[]},{"propositions":[],"lastnames":["Tooprakai"],"firstnames":["P."],"suffixes":[]},{"propositions":[],"lastnames":["Seripienlert"],"firstnames":["A."],"suffixes":[]},{"propositions":[],"lastnames":["Chuychai"],"firstnames":["P."],"suffixes":[]},{"propositions":[],"lastnames":["V","Usmanov"],"firstnames":["A."],"suffixes":[]},{"propositions":[],"lastnames":["Goldstein"],"firstnames":["M.","L."],"suffixes":[]},{"propositions":[],"lastnames":["McComas"],"firstnames":["D.","J."],"suffixes":[]},{"propositions":[],"lastnames":["Leske"],"firstnames":["R.","A."],"suffixes":[]},{"propositions":[],"lastnames":["Szalay"],"firstnames":["J.","R."],"suffixes":[]},{"propositions":[],"lastnames":["Joyce"],"firstnames":["C.","J."],"suffixes":[]},{"propositions":[],"lastnames":["Cummings"],"firstnames":["A.","C."],"suffixes":[]},{"propositions":[],"lastnames":["Roelof"],"firstnames":["E.","C."],"suffixes":[]},{"propositions":[],"lastnames":["Christian"],"firstnames":["E.","R."],"suffixes":[]},{"propositions":[],"lastnames":["Mewaldt"],"firstnames":["R.","A."],"suffixes":[]},{"propositions":[],"lastnames":["Labrador"],"firstnames":["A.","W."],"suffixes":[]},{"propositions":[],"lastnames":["Giacalone"],"firstnames":["J."],"suffixes":[]},{"propositions":[],"lastnames":["Schwadron"],"firstnames":["N.","A."],"suffixes":[]},{"propositions":[],"lastnames":["Mitchell"],"firstnames":["D.","G."],"suffixes":[]},{"propositions":[],"lastnames":["Hill"],"firstnames":["M.","E."],"suffixes":[]},{"propositions":[],"lastnames":["Wiedenbeck"],"firstnames":["M.","E."],"suffixes":[]},{"propositions":[],"lastnames":["Jr.","McNutt"],"firstnames":["R.","L."],"suffixes":[]},{"propositions":[],"lastnames":["I","Desai"],"firstnames":["M."],"suffixes":[]}],"year":"2021","note":"Publisher: Edp Sciences S A Type: Article tex.date-modified: 2022-04-12 11:34:55 +0100","bibtex":"@article{Chhiber2021,\n\ttitle = {Magnetic field line random walk and solar energetic particle path lengths {Stochastic} theory and {PSP}/{IS} circle dot {IS} observations},\n\tvolume = {650},\n\tissn = {0004-6361},\n\turl = {https://doi.org/10.1051/0004-6361/202039816},\n\tdoi = {10.1051/0004-6361/202039816},\n\tabstract = {Context. In 2020 May-June, six solar energetic ion events were observed by the Parker Solar Probe/IS circle dot IS instrument suite at approximate to 0.35 AU from the Sun. From standard velocity-dispersion analysis, the apparent ion path length is approximate to 0.625 AU at the onset of each event.},\n\tjournal = {Astronomy \\& Astrophysics},\n\tauthor = {Chhiber, R. and Matthaeus, W. H. and Cohen, C. M. S. and Ruffolo, D. and Sonsrettee, W. and Tooprakai, P. and Seripienlert, A. and Chuychai, P. and V Usmanov, A. and Goldstein, M. L. and McComas, D. J. and Leske, R. A. and Szalay, J. R. and Joyce, C. J. and Cummings, A. C. and Roelof, E. C. and Christian, E. R. and Mewaldt, R. A. and Labrador, A. W. and Giacalone, J. and Schwadron, N. A. and Mitchell, D. G. and Hill, M. E. and Wiedenbeck, M. E. and Jr. McNutt, R. L. and I Desai, M.},\n\tyear = {2021},\n\tnote = {Publisher: Edp Sciences S A\nType: Article\ntex.date-modified: 2022-04-12 11:34:55 +0100},\n}\n\n","author_short":["Chhiber, R.","Matthaeus, W. H.","Cohen, C. M. S.","Ruffolo, D.","Sonsrettee, W.","Tooprakai, P.","Seripienlert, A.","Chuychai, P.","V Usmanov, A.","Goldstein, M. L.","McComas, D. J.","Leske, R. A.","Szalay, J. R.","Joyce, C. J.","Cummings, A. C.","Roelof, E. C.","Christian, E. R.","Mewaldt, R. A.","Labrador, A. W.","Giacalone, J.","Schwadron, N. A.","Mitchell, D. G.","Hill, M. E.","Wiedenbeck, M. E.","Jr. McNutt, R. L.","I Desai, M."],"key":"Chhiber2021","id":"Chhiber2021","bibbaseid":"chhiber-matthaeus-cohen-ruffolo-sonsrettee-tooprakai-seripienlert-chuychai-etal-magneticfieldlinerandomwalkandsolarenergeticparticlepathlengthsstochastictheoryandpspiscircledotisobservations-2021","role":"author","urls":{"Paper":"https://doi.org/10.1051/0004-6361/202039816"},"metadata":{"authorlinks":{}},"html":""},"bibtype":"article","biburl":"https://bibbase.org/zotero/lloydwoodham","dataSources":["KswDSEBpD9sHPxkz4"],"keywords":[],"search_terms":["magnetic","field","line","random","walk","solar","energetic","particle","path","lengths","stochastic","theory","psp","circle","dot","observations","chhiber","matthaeus","cohen","ruffolo","sonsrettee","tooprakai","seripienlert","chuychai","v usmanov","goldstein","mccomas","leske","szalay","joyce","cummings","roelof","christian","mewaldt","labrador","giacalone","schwadron","mitchell","hill","wiedenbeck","jr. mcnutt","i desai"],"title":"Magnetic field line random walk and solar energetic particle path lengths Stochastic theory and PSP/IS circle dot IS observations","year":2021}