<resource xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://datacite.org/schema/kernel-4" xsi:schemaLocation="http://datacite.org/schema/kernel-4 http://schema.datacite.org/meta/kernel-4.1/metadata.xsd"><identifier identifierType="DOI">10.7910/DVN/BQNUZZ</identifier><creators><creator><creatorName nameType="Personal">Kamaletdinov, Sergey R.; Hutchinson, Ian H.; Vasko, Ivan Y.; Artemyev, Anton V.; Lotekar, Ajay; Mozer, Forrest</creatorName></creator></creators><titles><title>Spacecraft Observations and Theoretical Understanding of Slow Electron Holes</title></titles><publisher>Harvard Dataverse</publisher><publicationYear>2022</publicationYear><subjects><subject>Physics</subject><subject>condition</subject><subject>electron hole</subject><subject>local minimums</subject><subject>magnetospheric multi scale</subject><subject>slow electrons</subject><subject>velocity distribution functions</subject></subjects><dates><date dateType="Updated">2022-10-15</date></dates><resourceType resourceTypeGeneral="Dataset"/><sizes><size>14983706</size></sizes><formats><format>application/pdf</format></formats><version>2.0</version><rightsList><rights rightsURI="info:eu-repo/semantics/openAccess"/><rights/></rightsList><descriptions><description descriptionType="Abstract">We present Magnetospheric Multiscale observations showing large numbers of slow electron holes with speeds clustered near the local minimum of double-humped velocity distribution functions of background ions. Theoretical computations show that slow electron holes can avoid the acceleration that otherwise prevents their remaining slow only under these same circumstances. Although the origin of the slow electron holes is still elusive, the agreement between observation and theory about the conditions for their existence is remarkable.</description><description descriptionType="Other">&lt;a href="http://library.psfc.mit.edu/catalog/reports/2020/21ja/21ja048/abstract.php">PSFC REPORT PSFC/JA-21-48&lt;/a>&lt;br />&lt;br />None&lt;br />&lt;br />If this record does not contain the full text, then the manuscript has been embargoed by the publisher thus restricting open access for 12 to 24 months after publication.</description></descriptions><geoLocations/></resource>