Sodium variation in Geminid meteoroids from (3200) Phaethon
Sodium is a perfect indicator to investigate the volatility within meteoroid composition. Spectroscopic observations of the Geminid meteors were carried out using modern high sensitive large format CMOS cameras. 149 visible spectra of the Geminid meteors observed in 2017 and 2018 were analyzed by a...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Abe, Shinsuke [verfasserIn] |
|---|
| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2020transfer abstract |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: ENDOLOOP-ASSISTED TRANSORAL OUTLET REDUCTION: A PILOT CASE-CONTROL STUDY OF A NEW THERAPEUTIC INTERVENTION FOR WEIGHT REGAIN AFTER ROUX-EN-Y GASTRIC BYPASS - Mekaroonkamol, Parit ELSEVIER, 2023, Kidlington [u.a.] |
|---|---|
| Übergeordnetes Werk: |
volume:194 ; year:2020 ; pages:0 |
| Links: |
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| DOI / URN: |
10.1016/j.pss.2020.105040 |
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| 520 | |a Sodium is a perfect indicator to investigate the volatility within meteoroid composition. Spectroscopic observations of the Geminid meteors were carried out using modern high sensitive large format CMOS cameras. 149 visible spectra of the Geminid meteors observed in 2017 and 2018 were analyzed by a newly developed procedure. The variation of Na, Mg and Fe during meteor ablation in the atmosphere has been studied. Although sodium is depleted in ~ 80% of the Geminids, statistically significant variations of sodium in the Geminid meteors were found. It should be noted that Na depletion in the Geminid meteors increased with decreasing meteoroid size. A yearly variation of Na in the Geminid meteor streams was also found. Solar-heating age across the different parts of the meteoroids stream ejected from a parent active asteroid (3200) Phaethon having 0.14 AU small perihelion distance seems to the most likely explanation for the sodium variation and depletion. Surprisingly, three iron Geminid meteors were detected across the maximum of 2018 Geminids. | ||
| 520 | |a Sodium is a perfect indicator to investigate the volatility within meteoroid composition. Spectroscopic observations of the Geminid meteors were carried out using modern high sensitive large format CMOS cameras. 149 visible spectra of the Geminid meteors observed in 2017 and 2018 were analyzed by a newly developed procedure. The variation of Na, Mg and Fe during meteor ablation in the atmosphere has been studied. Although sodium is depleted in ~ 80% of the Geminids, statistically significant variations of sodium in the Geminid meteors were found. It should be noted that Na depletion in the Geminid meteors increased with decreasing meteoroid size. A yearly variation of Na in the Geminid meteor streams was also found. Solar-heating age across the different parts of the meteoroids stream ejected from a parent active asteroid (3200) Phaethon having 0.14 AU small perihelion distance seems to the most likely explanation for the sodium variation and depletion. Surprisingly, three iron Geminid meteors were detected across the maximum of 2018 Geminids. | ||
| 650 | 7 | |a Geminids |2 Elsevier | |
| 650 | 7 | |a Spectroscopy |2 Elsevier | |
| 650 | 7 | |a Meteors |2 Elsevier | |
| 650 | 7 | |a Meteoroids |2 Elsevier | |
| 650 | 7 | |a (3200) Phaethon |2 Elsevier | |
| 700 | 1 | |a Ogawa, Takumi |4 oth | |
| 700 | 1 | |a Maeda, Koji |4 oth | |
| 700 | 1 | |a Arai, Tomoko |4 oth | |
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10.1016/j.pss.2020.105040 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001222.pica (DE-627)ELV052270815 (ELSEVIER)S0032-0633(19)30496-9 DE-627 ger DE-627 rakwb eng 610 VZ 44.87 bkl Abe, Shinsuke verfasserin aut Sodium variation in Geminid meteoroids from (3200) Phaethon 2020transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Sodium is a perfect indicator to investigate the volatility within meteoroid composition. Spectroscopic observations of the Geminid meteors were carried out using modern high sensitive large format CMOS cameras. 149 visible spectra of the Geminid meteors observed in 2017 and 2018 were analyzed by a newly developed procedure. The variation of Na, Mg and Fe during meteor ablation in the atmosphere has been studied. Although sodium is depleted in ~ 80% of the Geminids, statistically significant variations of sodium in the Geminid meteors were found. It should be noted that Na depletion in the Geminid meteors increased with decreasing meteoroid size. A yearly variation of Na in the Geminid meteor streams was also found. Solar-heating age across the different parts of the meteoroids stream ejected from a parent active asteroid (3200) Phaethon having 0.14 AU small perihelion distance seems to the most likely explanation for the sodium variation and depletion. Surprisingly, three iron Geminid meteors were detected across the maximum of 2018 Geminids. Sodium is a perfect indicator to investigate the volatility within meteoroid composition. Spectroscopic observations of the Geminid meteors were carried out using modern high sensitive large format CMOS cameras. 149 visible spectra of the Geminid meteors observed in 2017 and 2018 were analyzed by a newly developed procedure. The variation of Na, Mg and Fe during meteor ablation in the atmosphere has been studied. Although sodium is depleted in ~ 80% of the Geminids, statistically significant variations of sodium in the Geminid meteors were found. It should be noted that Na depletion in the Geminid meteors increased with decreasing meteoroid size. A yearly variation of Na in the Geminid meteor streams was also found. Solar-heating age across the different parts of the meteoroids stream ejected from a parent active asteroid (3200) Phaethon having 0.14 AU small perihelion distance seems to the most likely explanation for the sodium variation and depletion. Surprisingly, three iron Geminid meteors were detected across the maximum of 2018 Geminids. Geminids Elsevier Spectroscopy Elsevier Meteors Elsevier Meteoroids Elsevier (3200) Phaethon Elsevier Ogawa, Takumi oth Maeda, Koji oth Arai, Tomoko oth Enthalten in Elsevier Science Mekaroonkamol, Parit ELSEVIER ENDOLOOP-ASSISTED TRANSORAL OUTLET REDUCTION: A PILOT CASE-CONTROL STUDY OF A NEW THERAPEUTIC INTERVENTION FOR WEIGHT REGAIN AFTER ROUX-EN-Y GASTRIC BYPASS 2023 Kidlington [u.a.] (DE-627)ELV010254102 volume:194 year:2020 pages:0 https://doi.org/10.1016/j.pss.2020.105040 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_66 GBV_ILN_91 GBV_ILN_165 GBV_ILN_234 44.87 Gastroenterologie VZ AR 194 2020 0 |
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10.1016/j.pss.2020.105040 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001222.pica (DE-627)ELV052270815 (ELSEVIER)S0032-0633(19)30496-9 DE-627 ger DE-627 rakwb eng 610 VZ 44.87 bkl Abe, Shinsuke verfasserin aut Sodium variation in Geminid meteoroids from (3200) Phaethon 2020transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Sodium is a perfect indicator to investigate the volatility within meteoroid composition. Spectroscopic observations of the Geminid meteors were carried out using modern high sensitive large format CMOS cameras. 149 visible spectra of the Geminid meteors observed in 2017 and 2018 were analyzed by a newly developed procedure. The variation of Na, Mg and Fe during meteor ablation in the atmosphere has been studied. Although sodium is depleted in ~ 80% of the Geminids, statistically significant variations of sodium in the Geminid meteors were found. It should be noted that Na depletion in the Geminid meteors increased with decreasing meteoroid size. A yearly variation of Na in the Geminid meteor streams was also found. Solar-heating age across the different parts of the meteoroids stream ejected from a parent active asteroid (3200) Phaethon having 0.14 AU small perihelion distance seems to the most likely explanation for the sodium variation and depletion. Surprisingly, three iron Geminid meteors were detected across the maximum of 2018 Geminids. Sodium is a perfect indicator to investigate the volatility within meteoroid composition. Spectroscopic observations of the Geminid meteors were carried out using modern high sensitive large format CMOS cameras. 149 visible spectra of the Geminid meteors observed in 2017 and 2018 were analyzed by a newly developed procedure. The variation of Na, Mg and Fe during meteor ablation in the atmosphere has been studied. Although sodium is depleted in ~ 80% of the Geminids, statistically significant variations of sodium in the Geminid meteors were found. It should be noted that Na depletion in the Geminid meteors increased with decreasing meteoroid size. A yearly variation of Na in the Geminid meteor streams was also found. Solar-heating age across the different parts of the meteoroids stream ejected from a parent active asteroid (3200) Phaethon having 0.14 AU small perihelion distance seems to the most likely explanation for the sodium variation and depletion. Surprisingly, three iron Geminid meteors were detected across the maximum of 2018 Geminids. Geminids Elsevier Spectroscopy Elsevier Meteors Elsevier Meteoroids Elsevier (3200) Phaethon Elsevier Ogawa, Takumi oth Maeda, Koji oth Arai, Tomoko oth Enthalten in Elsevier Science Mekaroonkamol, Parit ELSEVIER ENDOLOOP-ASSISTED TRANSORAL OUTLET REDUCTION: A PILOT CASE-CONTROL STUDY OF A NEW THERAPEUTIC INTERVENTION FOR WEIGHT REGAIN AFTER ROUX-EN-Y GASTRIC BYPASS 2023 Kidlington [u.a.] (DE-627)ELV010254102 volume:194 year:2020 pages:0 https://doi.org/10.1016/j.pss.2020.105040 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_66 GBV_ILN_91 GBV_ILN_165 GBV_ILN_234 44.87 Gastroenterologie VZ AR 194 2020 0 |
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10.1016/j.pss.2020.105040 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001222.pica (DE-627)ELV052270815 (ELSEVIER)S0032-0633(19)30496-9 DE-627 ger DE-627 rakwb eng 610 VZ 44.87 bkl Abe, Shinsuke verfasserin aut Sodium variation in Geminid meteoroids from (3200) Phaethon 2020transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Sodium is a perfect indicator to investigate the volatility within meteoroid composition. Spectroscopic observations of the Geminid meteors were carried out using modern high sensitive large format CMOS cameras. 149 visible spectra of the Geminid meteors observed in 2017 and 2018 were analyzed by a newly developed procedure. The variation of Na, Mg and Fe during meteor ablation in the atmosphere has been studied. Although sodium is depleted in ~ 80% of the Geminids, statistically significant variations of sodium in the Geminid meteors were found. It should be noted that Na depletion in the Geminid meteors increased with decreasing meteoroid size. A yearly variation of Na in the Geminid meteor streams was also found. Solar-heating age across the different parts of the meteoroids stream ejected from a parent active asteroid (3200) Phaethon having 0.14 AU small perihelion distance seems to the most likely explanation for the sodium variation and depletion. Surprisingly, three iron Geminid meteors were detected across the maximum of 2018 Geminids. Sodium is a perfect indicator to investigate the volatility within meteoroid composition. Spectroscopic observations of the Geminid meteors were carried out using modern high sensitive large format CMOS cameras. 149 visible spectra of the Geminid meteors observed in 2017 and 2018 were analyzed by a newly developed procedure. The variation of Na, Mg and Fe during meteor ablation in the atmosphere has been studied. Although sodium is depleted in ~ 80% of the Geminids, statistically significant variations of sodium in the Geminid meteors were found. It should be noted that Na depletion in the Geminid meteors increased with decreasing meteoroid size. A yearly variation of Na in the Geminid meteor streams was also found. Solar-heating age across the different parts of the meteoroids stream ejected from a parent active asteroid (3200) Phaethon having 0.14 AU small perihelion distance seems to the most likely explanation for the sodium variation and depletion. Surprisingly, three iron Geminid meteors were detected across the maximum of 2018 Geminids. Geminids Elsevier Spectroscopy Elsevier Meteors Elsevier Meteoroids Elsevier (3200) Phaethon Elsevier Ogawa, Takumi oth Maeda, Koji oth Arai, Tomoko oth Enthalten in Elsevier Science Mekaroonkamol, Parit ELSEVIER ENDOLOOP-ASSISTED TRANSORAL OUTLET REDUCTION: A PILOT CASE-CONTROL STUDY OF A NEW THERAPEUTIC INTERVENTION FOR WEIGHT REGAIN AFTER ROUX-EN-Y GASTRIC BYPASS 2023 Kidlington [u.a.] (DE-627)ELV010254102 volume:194 year:2020 pages:0 https://doi.org/10.1016/j.pss.2020.105040 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_66 GBV_ILN_91 GBV_ILN_165 GBV_ILN_234 44.87 Gastroenterologie VZ AR 194 2020 0 |
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10.1016/j.pss.2020.105040 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001222.pica (DE-627)ELV052270815 (ELSEVIER)S0032-0633(19)30496-9 DE-627 ger DE-627 rakwb eng 610 VZ 44.87 bkl Abe, Shinsuke verfasserin aut Sodium variation in Geminid meteoroids from (3200) Phaethon 2020transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Sodium is a perfect indicator to investigate the volatility within meteoroid composition. Spectroscopic observations of the Geminid meteors were carried out using modern high sensitive large format CMOS cameras. 149 visible spectra of the Geminid meteors observed in 2017 and 2018 were analyzed by a newly developed procedure. The variation of Na, Mg and Fe during meteor ablation in the atmosphere has been studied. Although sodium is depleted in ~ 80% of the Geminids, statistically significant variations of sodium in the Geminid meteors were found. It should be noted that Na depletion in the Geminid meteors increased with decreasing meteoroid size. A yearly variation of Na in the Geminid meteor streams was also found. Solar-heating age across the different parts of the meteoroids stream ejected from a parent active asteroid (3200) Phaethon having 0.14 AU small perihelion distance seems to the most likely explanation for the sodium variation and depletion. Surprisingly, three iron Geminid meteors were detected across the maximum of 2018 Geminids. Sodium is a perfect indicator to investigate the volatility within meteoroid composition. Spectroscopic observations of the Geminid meteors were carried out using modern high sensitive large format CMOS cameras. 149 visible spectra of the Geminid meteors observed in 2017 and 2018 were analyzed by a newly developed procedure. The variation of Na, Mg and Fe during meteor ablation in the atmosphere has been studied. Although sodium is depleted in ~ 80% of the Geminids, statistically significant variations of sodium in the Geminid meteors were found. It should be noted that Na depletion in the Geminid meteors increased with decreasing meteoroid size. A yearly variation of Na in the Geminid meteor streams was also found. Solar-heating age across the different parts of the meteoroids stream ejected from a parent active asteroid (3200) Phaethon having 0.14 AU small perihelion distance seems to the most likely explanation for the sodium variation and depletion. Surprisingly, three iron Geminid meteors were detected across the maximum of 2018 Geminids. Geminids Elsevier Spectroscopy Elsevier Meteors Elsevier Meteoroids Elsevier (3200) Phaethon Elsevier Ogawa, Takumi oth Maeda, Koji oth Arai, Tomoko oth Enthalten in Elsevier Science Mekaroonkamol, Parit ELSEVIER ENDOLOOP-ASSISTED TRANSORAL OUTLET REDUCTION: A PILOT CASE-CONTROL STUDY OF A NEW THERAPEUTIC INTERVENTION FOR WEIGHT REGAIN AFTER ROUX-EN-Y GASTRIC BYPASS 2023 Kidlington [u.a.] (DE-627)ELV010254102 volume:194 year:2020 pages:0 https://doi.org/10.1016/j.pss.2020.105040 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_66 GBV_ILN_91 GBV_ILN_165 GBV_ILN_234 44.87 Gastroenterologie VZ AR 194 2020 0 |
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10.1016/j.pss.2020.105040 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001222.pica (DE-627)ELV052270815 (ELSEVIER)S0032-0633(19)30496-9 DE-627 ger DE-627 rakwb eng 610 VZ 44.87 bkl Abe, Shinsuke verfasserin aut Sodium variation in Geminid meteoroids from (3200) Phaethon 2020transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Sodium is a perfect indicator to investigate the volatility within meteoroid composition. Spectroscopic observations of the Geminid meteors were carried out using modern high sensitive large format CMOS cameras. 149 visible spectra of the Geminid meteors observed in 2017 and 2018 were analyzed by a newly developed procedure. The variation of Na, Mg and Fe during meteor ablation in the atmosphere has been studied. Although sodium is depleted in ~ 80% of the Geminids, statistically significant variations of sodium in the Geminid meteors were found. It should be noted that Na depletion in the Geminid meteors increased with decreasing meteoroid size. A yearly variation of Na in the Geminid meteor streams was also found. Solar-heating age across the different parts of the meteoroids stream ejected from a parent active asteroid (3200) Phaethon having 0.14 AU small perihelion distance seems to the most likely explanation for the sodium variation and depletion. Surprisingly, three iron Geminid meteors were detected across the maximum of 2018 Geminids. Sodium is a perfect indicator to investigate the volatility within meteoroid composition. Spectroscopic observations of the Geminid meteors were carried out using modern high sensitive large format CMOS cameras. 149 visible spectra of the Geminid meteors observed in 2017 and 2018 were analyzed by a newly developed procedure. The variation of Na, Mg and Fe during meteor ablation in the atmosphere has been studied. Although sodium is depleted in ~ 80% of the Geminids, statistically significant variations of sodium in the Geminid meteors were found. It should be noted that Na depletion in the Geminid meteors increased with decreasing meteoroid size. A yearly variation of Na in the Geminid meteor streams was also found. Solar-heating age across the different parts of the meteoroids stream ejected from a parent active asteroid (3200) Phaethon having 0.14 AU small perihelion distance seems to the most likely explanation for the sodium variation and depletion. Surprisingly, three iron Geminid meteors were detected across the maximum of 2018 Geminids. Geminids Elsevier Spectroscopy Elsevier Meteors Elsevier Meteoroids Elsevier (3200) Phaethon Elsevier Ogawa, Takumi oth Maeda, Koji oth Arai, Tomoko oth Enthalten in Elsevier Science Mekaroonkamol, Parit ELSEVIER ENDOLOOP-ASSISTED TRANSORAL OUTLET REDUCTION: A PILOT CASE-CONTROL STUDY OF A NEW THERAPEUTIC INTERVENTION FOR WEIGHT REGAIN AFTER ROUX-EN-Y GASTRIC BYPASS 2023 Kidlington [u.a.] (DE-627)ELV010254102 volume:194 year:2020 pages:0 https://doi.org/10.1016/j.pss.2020.105040 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_66 GBV_ILN_91 GBV_ILN_165 GBV_ILN_234 44.87 Gastroenterologie VZ AR 194 2020 0 |
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English |
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Enthalten in ENDOLOOP-ASSISTED TRANSORAL OUTLET REDUCTION: A PILOT CASE-CONTROL STUDY OF A NEW THERAPEUTIC INTERVENTION FOR WEIGHT REGAIN AFTER ROUX-EN-Y GASTRIC BYPASS Kidlington [u.a.] volume:194 year:2020 pages:0 |
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Enthalten in ENDOLOOP-ASSISTED TRANSORAL OUTLET REDUCTION: A PILOT CASE-CONTROL STUDY OF A NEW THERAPEUTIC INTERVENTION FOR WEIGHT REGAIN AFTER ROUX-EN-Y GASTRIC BYPASS Kidlington [u.a.] volume:194 year:2020 pages:0 |
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ENDOLOOP-ASSISTED TRANSORAL OUTLET REDUCTION: A PILOT CASE-CONTROL STUDY OF A NEW THERAPEUTIC INTERVENTION FOR WEIGHT REGAIN AFTER ROUX-EN-Y GASTRIC BYPASS |
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Solar-heating age across the different parts of the meteoroids stream ejected from a parent active asteroid (3200) Phaethon having 0.14 AU small perihelion distance seems to the most likely explanation for the sodium variation and depletion. 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ENDOLOOP-ASSISTED TRANSORAL OUTLET REDUCTION: A PILOT CASE-CONTROL STUDY OF A NEW THERAPEUTIC INTERVENTION FOR WEIGHT REGAIN AFTER ROUX-EN-Y GASTRIC BYPASS |
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ENDOLOOP-ASSISTED TRANSORAL OUTLET REDUCTION: A PILOT CASE-CONTROL STUDY OF A NEW THERAPEUTIC INTERVENTION FOR WEIGHT REGAIN AFTER ROUX-EN-Y GASTRIC BYPASS |
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Sodium variation in Geminid meteoroids from (3200) Phaethon |
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ENDOLOOP-ASSISTED TRANSORAL OUTLET REDUCTION: A PILOT CASE-CONTROL STUDY OF A NEW THERAPEUTIC INTERVENTION FOR WEIGHT REGAIN AFTER ROUX-EN-Y GASTRIC BYPASS |
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sodium variation in geminid meteoroids from (3200) phaethon |
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Sodium variation in Geminid meteoroids from (3200) Phaethon |
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Sodium is a perfect indicator to investigate the volatility within meteoroid composition. Spectroscopic observations of the Geminid meteors were carried out using modern high sensitive large format CMOS cameras. 149 visible spectra of the Geminid meteors observed in 2017 and 2018 were analyzed by a newly developed procedure. The variation of Na, Mg and Fe during meteor ablation in the atmosphere has been studied. Although sodium is depleted in ~ 80% of the Geminids, statistically significant variations of sodium in the Geminid meteors were found. It should be noted that Na depletion in the Geminid meteors increased with decreasing meteoroid size. A yearly variation of Na in the Geminid meteor streams was also found. Solar-heating age across the different parts of the meteoroids stream ejected from a parent active asteroid (3200) Phaethon having 0.14 AU small perihelion distance seems to the most likely explanation for the sodium variation and depletion. Surprisingly, three iron Geminid meteors were detected across the maximum of 2018 Geminids. |
| abstractGer |
Sodium is a perfect indicator to investigate the volatility within meteoroid composition. Spectroscopic observations of the Geminid meteors were carried out using modern high sensitive large format CMOS cameras. 149 visible spectra of the Geminid meteors observed in 2017 and 2018 were analyzed by a newly developed procedure. The variation of Na, Mg and Fe during meteor ablation in the atmosphere has been studied. Although sodium is depleted in ~ 80% of the Geminids, statistically significant variations of sodium in the Geminid meteors were found. It should be noted that Na depletion in the Geminid meteors increased with decreasing meteoroid size. A yearly variation of Na in the Geminid meteor streams was also found. Solar-heating age across the different parts of the meteoroids stream ejected from a parent active asteroid (3200) Phaethon having 0.14 AU small perihelion distance seems to the most likely explanation for the sodium variation and depletion. Surprisingly, three iron Geminid meteors were detected across the maximum of 2018 Geminids. |
| abstract_unstemmed |
Sodium is a perfect indicator to investigate the volatility within meteoroid composition. Spectroscopic observations of the Geminid meteors were carried out using modern high sensitive large format CMOS cameras. 149 visible spectra of the Geminid meteors observed in 2017 and 2018 were analyzed by a newly developed procedure. The variation of Na, Mg and Fe during meteor ablation in the atmosphere has been studied. Although sodium is depleted in ~ 80% of the Geminids, statistically significant variations of sodium in the Geminid meteors were found. It should be noted that Na depletion in the Geminid meteors increased with decreasing meteoroid size. A yearly variation of Na in the Geminid meteor streams was also found. Solar-heating age across the different parts of the meteoroids stream ejected from a parent active asteroid (3200) Phaethon having 0.14 AU small perihelion distance seems to the most likely explanation for the sodium variation and depletion. Surprisingly, three iron Geminid meteors were detected across the maximum of 2018 Geminids. |
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Sodium variation in Geminid meteoroids from (3200) Phaethon |
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