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Browsing by Author "Chasapis, A."

Browsing by Author "Chasapis, A."

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  • Chhiber, Rohit; Goldstein, M. L.; Maruca, B. A.; Chasapis, A.; Matthaeus, W. H.; Ruffolo, D.; Bandyopadhyay, R.; Parashar, T. N.; Qudsi, R.; de Wit, T. Dudok; Bale, S. D.; Bonnell, John W.; Goetz, K.; Harvey, P. R.; MacDowall, R. J.; Malaspina, D.; Pulupa, M.; Kasper, Justin C.; Korreck, Kelly E.; Case, Anthony W.; Stevens, Michael L.; Whittlesey, P.; Larson, D.; Livi, R.; Velli, M.; Raouafi, N. (2020)
    During the Parker Solar Probe&#39;s (PSP) first perihelion pass, the spacecraft reached within a heliocentric distance of ~37 R<SUB>?</SUB> and observed numerous magnetic and flow structures characterized by sharp gradients. ...
  • Bandyopadhyay, Riddhi; Goldstein, M. L.; Maruca, B. A.; Matthaeus, W. H.; Parashar, T. N.; Ruffolo, D.; Chhiber, R.; Usmanov, A.; Chasapis, A.; Qudsi, R.; Bale, Stuart D.; Bonnell, John W.; Dudok de Wit, Thierry; Goetz, Keith; Harvey, Peter R.; MacDowall, Robert J.; Malaspina, David M.; Pulupa, Marc; Kasper, Justin C.; Korreck, Kelly E.; Case, Anthony W.; Stevens, Michael; Whittlesey, P.; Larson, D.; Livi, R.; Klein, K. G.; Velli, M.; Raouafi, N. (2020)
    Direct evidence of an inertial-range turbulent energy cascade has been provided by spacecraft observations in heliospheric plasmas. In the solar wind, the average value of the derived heating rate near 1 au is $\sim ...
  • Goldstein, Melvyn; Ruffolo, D.; Matthaeus, W. H.; Chhiber, R.; Usmanov, A. V.; Yang, Y.; Bandyopadhyay, R.; Parashar, T. N.; DeForest, E.; Wan, M.; Chasapis, A.; Maruca, B. A.; Velli, M.; Kasper, Justin C. (2020)
  • Bowen, T. A.; Bale, S. D.; Bandyopadhyay, R.; Bonnell, J. W.; Case, Anthony; Chasapis, A.; Chen, C. H. K.; Curry, S.; Dudok de Wit, T.; Goetz, K.; Goodrich, K.; Gruesbeck, J.; Halekas, J.; Harvey, P. R.; Howes, G. G.; Kasper, J. C.; Korreck, Kelly; Larson, D.; Livi, R.; MacDowall, R. J.; Malaspina, D. M.; Mallet, A.; McManus, M. D.; Page, B.; Pulupa, M.; Raouafi, N.; Stevens, Michael L.; Whittlesey, P. (2021)
    While not specifically designed as a planetary mission, NASA&#39;s Parker Solar Probe (PSP) mission uses a series of Venus gravity assists (VGAs) in order to reduce its perihelion distance. These orbital maneuvers provide ...
  • Parashar, T. N.; Goldstein, M. L.; Maruca, B. A.; Matthaeus, W. H.; Ruffolo, D.; Bandyopadhyay, R.; Chhiber, R.; Chasapis, A.; Qudsi, R.; Vech, D.; Roberts, D. A.; Bale, S. D.; Bonnell, John W.; de Wit, T. Dudok; Goetz, K.; Harvey, P. R.; MacDowall, R. J.; Malaspina, D.; Pulupa, M.; Kasper, Justin C.; Korreck, Kelly E.; Case, Anthony W.; Stevens, Michael; Whittlesey, P.; Larson, D.; Livi, R.; Velli, M.; Raouafi, N. (2020)
    The solar wind shows periods of highly Alfvénic activity, where velocity fluctuations and magnetic fluctuations are aligned or antialigned with each other. It is generally agreed that solar wind plasma velocity and magnetic ...
  • Bandyopadhyay, Riddhi; 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, J. R.; Joyce, C. J.; Giacalone, J.; Schwadron, N. A.; Mitchell, D. G.; Hill, M. E.; Wiedenbeck, M. E.; McNutt, R. L., Jr.; Desai, M. I.; Bale, Stuart D.; Bonnell, John W.; de Wit, Thierry Dudok; Goetz, Keith; Harvey, Peter R.; MacDowall, Robert J.; Malaspina, David M.; Pulupa, Marc; Velli, M.; Kasper, Justin C.; Korreck, Kelly E.; Stevens, Michael; Case, Anthony W.; Raouafi, N. (2020)
    Observations at 1 au have confirmed that enhancements in measured energetic-particle (EP) fluxes are statistically associated with &quot;rough&quot; magnetic fields, i.e., fields with atypically large spatial derivatives ...
  • Qudsi, R. A.; Maruca, B. A.; Matthaeus, W. H.; Parashar, T. N.; Bandyopadhyay, Riddhi; Chhiber, R.; Chasapis, A.; Goldstein, Melvyn L.; Bale, S. D.; Bonnell, J. W.; Dudok de Wit, T.; Goetz, K.; Harvey, P. R.; MacDowall, R. J.; Malaspina, D.; Pulupa, M.; Kasper, Justin C.; Korreck, Kelly E.; Case, Anthony W.; Stevens, Michael; Whittlesey, P.; Larson, D.; Livi, R.; Velli, M.; Raouafi, N. (2020)
    The solar wind proton temperature at 1 au has been found to be correlated with small-scale intermittent magnetic structures, i.e., regions with enhanced temperature are associated with coherent structures, such as current ...

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