{"data":{"id":"10.6084/m9.figshare.1282525","type":"dois","attributes":{"doi":"10.6084/m9.figshare.1282525","prefix":"10.6084","suffix":"m9.figshare.1282525","identifiers":[],"alternateIdentifiers":[],"creators":[{"name":"Sochi, Taha","nameType":"Personal","givenName":"Taha","familyName":"Sochi","affiliation":[],"nameIdentifiers":[]}],"titles":[{"title":"Hydrogen emission \u0026amp; recombination coefficients with kappa electron distribution"}],"publisher":"figshare","container":{},"publicationYear":2014,"subjects":[{"subject":"Atomic Physics"},{"subject":"Interstellar and Intergalactic Matter"},{"subject":"20104 Galactic Astronomy","subjectScheme":"FOR"},{"subject":"FOS: Physical sciences","schemeUri":"http://www.oecd.org/science/inno/38235147.pdf","subjectScheme":"Fields of Science and Technology (FOS)"},{"subject":"FOS: Physical sciences","subjectScheme":"Fields of Science and Technology (FOS)"},{"subject":"Cosmology"},{"subject":"Stellar Astronomy"},{"subject":"Stars, Variable Stars"},{"subject":"Astrophysics"},{"subject":"Solar System, Solar Physics, Planets and Exoplanets"},{"subject":"Extragalactic Astronomy"}],"contributors":[],"dates":[{"date":"2014-12-31","dateType":"Created"},{"date":"2014-12-31","dateType":"Updated"},{"date":"2014","dateType":"Issued"}],"language":null,"types":{"ris":"DATA","bibtex":"misc","citeproc":"dataset","schemaOrg":"Dataset","resourceType":"Dataset","resourceTypeGeneral":"Dataset"},"relatedIdentifiers":[],"relatedItems":[],"sizes":["97722755 Bytes"],"formats":[],"version":null,"rightsList":[{"rights":"Creative Commons Attribution 4.0 International","rightsUri":"https://creativecommons.org/licenses/by/4.0/legalcode","schemeUri":"https://spdx.org/licenses/","rightsIdentifier":"cc-by-4.0","rightsIdentifierScheme":"SPDX"}],"descriptions":[{"description":"This list provides an extensive data set for the emission and total recombination coefficients of hydrogen and total recombination coefficients to the 2s two-photon transitions with a kappa electron energy distribution rather than the more traditional Maxwell-Boltzmann distribution. The data are mainly relevant to thin and relatively cold plasma found in planetary nebulae and H II regions. The data set is complementary to previous data sets provided by Hummer and Storey and Storey and Hummer under a Maxwell-Boltzmann distribution assumption based on thermodynamic equilibrium. The data set is structured as a function of electron number density, temperature and kappa. An interactive fortran 77 and C++ data servers are also provided as an accessory to probe the data and obtain Lagrange-interpolated values in all three variables between the explicitly given values.","descriptionType":"Abstract"}],"geoLocations":[],"fundingReferences":[],"xml":"PD94bWwgdmVyc2lvbj0iMS4wIiBlbmNvZGluZz0iVVRGLTgiPz4KPHJlc291cmNlIHhtbG5zPSJodHRwOi8vZGF0YWNpdGUub3JnL3NjaGVtYS9rZXJuZWwtNCIgeG1sbnM6eHNpPSJodHRwOi8vd3d3LnczLm9yZy8yMDAxL1hNTFNjaGVtYS1pbnN0YW5jZSIgeHNpOnNjaGVtYUxvY2F0aW9uPSJodHRwOi8vZGF0YWNpdGUub3JnL3NjaGVtYS9rZXJuZWwtNCBodHRwOi8vc2NoZW1hLmRhdGFjaXRlLm9yZy9tZXRhL2tlcm5lbC00LjEvbWV0YWRhdGEueHNkIj4KICA8aWRlbnRpZmllciBpZGVudGlmaWVyVHlwZT0iRE9JIj4xMC42MDg0L005LkZJR1NIQVJFLjEyODI1MjU8L2lkZW50aWZpZXI+CiAgPGNyZWF0b3JzPgogICAgPGNyZWF0b3I+CiAgICAgIDxjcmVhdG9yTmFtZT5UYWhhIFNvY2hpPC9jcmVhdG9yTmFtZT4KICAgIDwvY3JlYXRvcj4KICA8L2NyZWF0b3JzPgogIDx0aXRsZXM+CiAgICA8dGl0bGU+SHlkcm9nZW4gZW1pc3Npb24gJmFtcDsgcmVjb21iaW5hdGlvbiBjb2VmZmljaWVudHMgd2l0aCBrYXBwYSBlbGVjdHJvbiBkaXN0cmlidXRpb248L3RpdGxlPgogIDwvdGl0bGVzPgogIDxkZXNjcmlwdGlvbnM+CiAgICA8ZGVzY3JpcHRpb24gZGVzY3JpcHRpb25UeXBlPSJBYnN0cmFjdCI+Jmx0O3AmZ3Q7VGhpcyBsaXN0IHByb3ZpZGVzIGFuIGV4dGVuc2l2ZSBkYXRhIHNldCBmb3IgdGhlIGVtaXNzaW9uIGFuZCB0b3RhbCByZWNvbWJpbmF0aW9uIGNvZWZmaWNpZW50cyBvZiBoeWRyb2dlbiBhbmQgdG90YWwgcmVjb21iaW5hdGlvbiBjb2VmZmljaWVudHMgdG8gdGhlIDJzIHR3by1waG90b24gdHJhbnNpdGlvbnMgd2l0aCBhIGthcHBhIGVsZWN0cm9uIGVuZXJneSBkaXN0cmlidXRpb24gcmF0aGVyIHRoYW4gdGhlIG1vcmUgdHJhZGl0aW9uYWwgTWF4d2VsbC1Cb2x0em1hbm4gZGlzdHJpYnV0aW9uLiBUaGUgZGF0YSBhcmUgbWFpbmx5IHJlbGV2YW50IHRvIHRoaW4gYW5kIHJlbGF0aXZlbHkgY29sZCBwbGFzbWEgZm91bmQgaW4gcGxhbmV0YXJ5IG5lYnVsYWUgYW5kIEggSUkgcmVnaW9ucy4gVGhlIGRhdGEgc2V0IGlzIGNvbXBsZW1lbnRhcnkgdG8gcHJldmlvdXMgZGF0YSBzZXRzIHByb3ZpZGVkIGJ5IEh1bW1lciBhbmQgU3RvcmV5IGFuZCBTdG9yZXkgYW5kIEh1bW1lciB1bmRlciBhIE1heHdlbGwtQm9sdHptYW5uIGRpc3RyaWJ1dGlvbiBhc3N1bXB0aW9uIGJhc2VkIG9uIHRoZXJtb2R5bmFtaWMgZXF1aWxpYnJpdW0uIFRoZSBkYXRhIHNldCBpcyBzdHJ1Y3R1cmVkIGFzIGEgZnVuY3Rpb24gb2YgZWxlY3Ryb24gbnVtYmVyIGRlbnNpdHksIHRlbXBlcmF0dXJlIGFuZCBrYXBwYS4gQW4gaW50ZXJhY3RpdmUgZm9ydHJhbiA3NyBhbmQgQysrIGRhdGEgc2VydmVycyBhcmUgYWxzbyBwcm92aWRlZCBhcyBhbiBhY2Nlc3NvcnkgdG8gcHJvYmUgdGhlIGRhdGEgYW5kIG9idGFpbiBMYWdyYW5nZS1pbnRlcnBvbGF0ZWQgdmFsdWVzIGluIGFsbCB0aHJlZSB2YXJpYWJsZXMgYmV0d2VlbiB0aGUgZXhwbGljaXRseSBnaXZlbiB2YWx1ZXMuJmx0Oy9wJmd0OzwvZGVzY3JpcHRpb24+CiAgPC9kZXNjcmlwdGlvbnM+CiAgPHN1YmplY3RzPgogICAgPHN1YmplY3Q+QXRvbWljIFBoeXNpY3M8L3N1YmplY3Q+CiAgICA8c3ViamVjdD5JbnRlcnN0ZWxsYXIgYW5kIEludGVyZ2FsYWN0aWMgTWF0dGVyPC9zdWJqZWN0PgogICAgPHN1YmplY3Qgc2NoZW1lVVJJPSJodHRwOi8vd3d3LmFicy5nb3YuYXUvYXVzc3RhdHMvYWJzQC5uc2YvMC82QkI0MjdBQjk2OTZDMjI1Q0EyNTc0MTgwMDA0NDYzRSIgc3ViamVjdFNjaGVtZT0iRk9SIj4yMDEwNCBHYWxhY3RpYyBBc3Ryb25vbXk8L3N1YmplY3Q+CiAgICA8c3ViamVjdD5Db3Ntb2xvZ3k8L3N1YmplY3Q+CiAgICA8c3ViamVjdD5TdGVsbGFyIEFzdHJvbm9teTwvc3ViamVjdD4KICAgIDxzdWJqZWN0PlN0YXJzLCBWYXJpYWJsZSBTdGFyczwvc3ViamVjdD4KICAgIDxzdWJqZWN0PkFzdHJvcGh5c2ljczwvc3ViamVjdD4KICAgIDxzdWJqZWN0PlNvbGFyIFN5c3RlbSwgU29sYXIgUGh5c2ljcywgUGxhbmV0cyBhbmQgRXhvcGxhbmV0czwvc3ViamVjdD4KICAgIDxzdWJqZWN0PkV4dHJhZ2FsYWN0aWMgQXN0cm9ub215PC9zdWJqZWN0PgogIDwvc3ViamVjdHM+CiAgPHB1Ymxpc2hlcj5maWdzaGFyZTwvcHVibGlzaGVyPgogIDxwdWJsaWNhdGlvblllYXI+MjAxNDwvcHVibGljYXRpb25ZZWFyPgogIDxkYXRlcz4KICAgIDxkYXRlIGRhdGVUeXBlPSJDcmVhdGVkIj4yMDE0LTEyLTMxPC9kYXRlPgogICAgPGRhdGUgZGF0ZVR5cGU9IlVwZGF0ZWQiPjIwMTQtMTItMzE8L2RhdGU+CiAgPC9kYXRlcz4KICA8cmVzb3VyY2VUeXBlIHJlc291cmNlVHlwZUdlbmVyYWw9IkRhdGFzZXQiPkRhdGFzZXQ8L3Jlc291cmNlVHlwZT4KICA8c2l6ZXM+CiAgICA8c2l6ZT45NzcyMjc1NSBCeXRlczwvc2l6ZT4KICA8L3NpemVzPgogIDxyaWdodHNMaXN0PgogICAgPHJpZ2h0cyByaWdodHNVUkk9Imh0dHBzOi8vY3JlYXRpdmVjb21tb25zLm9yZy9saWNlbnNlcy9ieS80LjAvIj5DQyBCWSA0LjA8L3JpZ2h0cz4KICA8L3JpZ2h0c0xpc3Q+CjwvcmVzb3VyY2U+","url":"https://figshare.com/articles/dataset/Hydrogen_emission_amp_recombination_coefficients_with_kappa_electron_distribution/1282525","contentUrl":null,"metadataVersion":1,"schemaVersion":"http://datacite.org/schema/kernel-4","source":"mds","isActive":true,"state":"findable","reason":null,"viewCount":0,"viewsOverTime":[],"downloadCount":0,"downloadsOverTime":[],"referenceCount":0,"citationCount":0,"citationsOverTime":[],"partCount":0,"partOfCount":0,"versionCount":0,"versionOfCount":0,"created":"2014-12-31T18:02:27.000Z","registered":"2014-12-31T18:02:29.000Z","published":"2014","updated":"2020-09-04T19:45:50.000Z"},"relationships":{"client":{"data":{"id":"figshare.ars","type":"clients"}},"provider":{"data":{"id":"otjm","type":"providers"}},"media":{"data":{"id":"10.6084/m9.figshare.1282525","type":"media"}},"references":{"data":[]},"citations":{"data":[]},"parts":{"data":[]},"partOf":{"data":[]},"versions":{"data":[]},"versionOf":{"data":[]}}}}