| 1. Identity statement | ||||
| Reference Type | Journal Article | |||
| Site | mtc-m21c.sid.inpe.br | |||
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S | |||
| Identifier | 8JMKD3MGP3W34R/42JAMPS | |||
| Repository | sid.inpe.br/mtc-m21c/2020/05.29.11.19 (restricted access) | |||
| Last Update | 2020:05.29.11.19.32 (UTC) simone | |||
| Metadata Repository | sid.inpe.br/mtc-m21c/2020/05.29.11.19.32 | |||
| Metadata Last Update | 2022:01.04.01.35.10 (UTC) administrator | |||
| DOI | 10.1016/j.asr.2020.03.036 | |||
| ISSN | 0273-1177 1879-1948 | |||
| Citation Key | EcherBolzFran:2020:UlObEc | |||
| Title | Statistical analysis of solar wind parameter variation with heliospheric distance: Ulysses observations in the ecliptic plane  | |||
| Year | 2020 | |||
| Month | June | |||
| Access Date | 2024, May 16 | |||
| Type of Work | journal article | |||
| Secondary Type | PRE PI | |||
| Number of Files | 1 | |||
| Size | 2580 KiB | |||
| 2. Context | ||||
| Author | 1 Echer, Ezequiel 2 Bolzan, Maurício J. A. 3 Franco, Adriane Marques de Souza | |||
| Resume Identifier | 1 8JMKD3MGP5W/3C9JH3D | |||
| Group | 1 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 2 3 YYY-CGCEA-INPE-MCTIC-GOV-BR | |||
| Affiliation | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 Universidade Federal de Jataí 3 Instituto Nacional de Pesquisas Espaciais (INPE) | |||
| Author e-Mail Address | 1 ezequiel.echer@inpe.br 2 mauricio.bolzam@cnpq.br | |||
| Journal | Advances in Space Research | |||
| Volume | 65 | |||
| Number | 12 | |||
| Pages | 2846-2856 | |||
| Secondary Mark | B1_INTERDISCIPLINAR B1_GEOCIÊNCIAS B1_ENGENHARIAS_IV B1_ENGENHARIAS_III B1_BIODIVERSIDADE B3_CIÊNCIA_DA_COMPUTAÇÃO B4_ASTRONOMIA_/_FÍSICA C_CIÊNCIAS_BIOLÓGICAS_I | |||
| History (UTC) | 2020-05-29 11:19:32 :: simone -> administrator :: 2020-05-29 11:19:33 :: administrator -> simone :: 2020 2020-05-29 11:20:05 :: simone -> administrator :: 2020 2022-01-04 01:35:10 :: administrator -> simone :: 2020 | |||
| 3. Content and structure | ||||
| Is the master or a copy? | is the master | |||
| Content Stage | completed | |||
| Transferable | 1 | |||
| Content Type | External Contribution | |||
| Version Type | publisher | |||
| Keywords | Solar wind turbulence Ulysses spacecraft Kurtosis technique Wavelet analysis | |||
| Abstract | The interplanetary magnetic field magnitude B-o, proton density N-p and solar wind speed V, data from Ulysses spacecraft during its interplanetary cruise interval from Earth to Jupiter, from 18 November 1990 to 31 January 1992, are analyzed in this study. Statistical and wavelet techniques are employed to characterize some properties from the solar wind parameters near the ecliptic plane and their dependence with radial distance. The results from kurtosis analysis showed that the three solar wind parameters (B-o, and N-p and V-sw) presented a decrease of this statistical quantity with the increase of scales, indicating that these variables are intermittent in short time scales. Further, the kurtosis parameter presented an increase in all scales around 2-3 AU distance range that corresponds to a solar wind regime transition. It was noted that the interplanetary medium was dominated by solar transients (interplanetary coronal mass ejections) until the middle of 1991. Afterwards a more stable pattern of corotating interaction regions arose. Furthermore, the probability distribution functions presented a spreading shape due to the occurrence of intermittence. In order to study the temporal variability of the solar wind parameters, the wavelet approach was used. The following major periodicities were found for the three solar wind variables studied: similar to 13, similar to 26, and similar to 83-88 days. It was noted that the similar to 13 day periods presented strong spectral power in the 2 to 4 AU range, where the solar wind was dominated by ICME transients. On the other hand, the 26 day period shows higher spectral power for distances higher than 4 AU, where the interplanetary space is more dominated by CIRs. Thus, it was found in this paper a significant dependence of solar wind parameters on radial heliocentric distance which can be accounted by the dynamical evolution of solar wind structures with distance. | |||
| Area | CEA | |||
| Arrangement 1 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Statistical analysis of... | |||
| Arrangement 2 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > YYY-PCI-CGCEA > Statistical analysis of... | |||
| doc Directory Content | access | |||
| source Directory Content | there are no files | |||
| agreement Directory Content |
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| 4. Conditions of access and use | ||||
| Language | en | |||
| Target File | echer_statistical.pdf | |||
| User Group | simone | |||
| Reader Group | administrator simone | |||
| Visibility | shown | |||
| Archiving Policy | denypublisher denyfinaldraft24 | |||
| Read Permission | deny from all and allow from 150.163 | |||
| Update Permission | not transferred | |||
| 5. Allied materials | ||||
| Next Higher Units | 8JMKD3MGPCW/3EU29DP 8JMKD3MGPCW/4467GD8 | |||
| Citing Item List | sid.inpe.br/mtc-m21/2012/07.13.14.45.47 4 sid.inpe.br/bibdigital/2013/10.01.22.11 3 sid.inpe.br/bibdigital/2021/02.11.01.58 3 | |||
| Dissemination | WEBSCI; PORTALCAPES; COMPENDEX; SCOPUS. | |||
| Host Collection | urlib.net/www/2017/11.22.19.04 | |||
| 6. Notes | ||||
| Empty Fields | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url | |||
| 7. Description control | ||||
| e-Mail (login) | simone | |||
| update | ||||