MAVEN SupraThermal and Thermal Ion Compostion (STATIC) Instrument
The MAVEN SupraThermal And Thermal Ion Compostion (STATIC) instrument is designed to measure the ion composition and distribution function of the cold Martian ionosphere, the heated suprathermal tail of this plasma in the upper ionosphere, and the pickup ions accelerated by solar wind electric field...
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| Veröffentlicht in: | Space science reviews 2015-12, Vol.195 (1-4), p.199-256 |
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| creator | McFadden, J. P. Kortmann, O. Curtis, D. Dalton, G. Johnson, G. Abiad, R. Sterling, R. Hatch, K. Berg, P. Tiu, C. Gordon, D. Heavner, S. Robinson, M. Marckwordt, M. Lin, R. Jakosky, B. |
| description | The MAVEN SupraThermal And Thermal Ion Compostion (STATIC) instrument is designed to measure the ion composition and distribution function of the cold Martian ionosphere, the heated suprathermal tail of this plasma in the upper ionosphere, and the pickup ions accelerated by solar wind electric fields. STATIC operates over an energy range of 0.1 eV up to 30 keV, with a base time resolution of 4 seconds. The instrument consists of a toroidal “top hat” electrostatic analyzer with a
360
∘
×
90
∘
field-of-view, combined with a time-of-flight (TOF) velocity analyzer with
22.5
∘
resolution in the detection plane. The TOF combines a
−
15
kV
acceleration voltage with ultra-thin carbon foils to resolve
H
+
,
He
+
+
,
He
+
,
O
+
,
O
2
+
, and
CO
2
+
ions. Secondary electrons from carbon foils are detected by microchannel plate detectors and binned into a variety of data products with varying energy, mass, angle, and time resolution. To prevent detector saturation when measuring cold ram ions at periapsis (
∼
10
1
1
eV/cm
2
s
sr
eV
), while maintaining adequate sensitivity to resolve tenuous pickup ions at apoapsis (
∼
10
3
eV/cm
2
s
sr
eV
), the sensor includes both mechanical and electrostatic attenuators that increase the dynamic range by a factor of
10
3
. This paper describes the instrument hardware, including several innovative improvements over previous TOF sensors, the ground calibrations of the sensor, the data products generated by the experiment, and some early measurements during cruise phase to Mars. |
| doi_str_mv | 10.1007/s11214-015-0175-6 |
| format | Article |
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360
∘
×
90
∘
field-of-view, combined with a time-of-flight (TOF) velocity analyzer with
22.5
∘
resolution in the detection plane. The TOF combines a
−
15
kV
acceleration voltage with ultra-thin carbon foils to resolve
H
+
,
He
+
+
,
He
+
,
O
+
,
O
2
+
, and
CO
2
+
ions. Secondary electrons from carbon foils are detected by microchannel plate detectors and binned into a variety of data products with varying energy, mass, angle, and time resolution. To prevent detector saturation when measuring cold ram ions at periapsis (
∼
10
1
1
eV/cm
2
s
sr
eV
), while maintaining adequate sensitivity to resolve tenuous pickup ions at apoapsis (
∼
10
3
eV/cm
2
s
sr
eV
), the sensor includes both mechanical and electrostatic attenuators that increase the dynamic range by a factor of
10
3
. This paper describes the instrument hardware, including several innovative improvements over previous TOF sensors, the ground calibrations of the sensor, the data products generated by the experiment, and some early measurements during cruise phase to Mars.</description><identifier>ISSN: 0038-6308</identifier><identifier>EISSN: 1572-9672</identifier><identifier>DOI: 10.1007/s11214-015-0175-6</identifier><language>eng</language><publisher>Dordrecht: Springer Netherlands</publisher><subject>Aerospace Technology and Astronautics ; Analyzers (electric) ; Astrophysics and Astroparticles ; Carbon ; Composting ; Detectors ; Electric fields ; Electrostatics ; Foils ; Ionosphere ; Ions ; Mars ; Physics ; Physics and Astronomy ; Planetology ; Sensors ; Space exploration ; Space Exploration and Astronautics ; Space Sciences (including Extraterrestrial Physics ; Spacecraft</subject><ispartof>Space science reviews, 2015-12, Vol.195 (1-4), p.199-256</ispartof><rights>The Author(s) 2015</rights><rights>Springer Science+Business Media Dordrecht 2015</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c561t-9cc6ea4b58fc26e2359d11a2084df69b269375cf1a99a110ef6cff2979f210573</citedby><cites>FETCH-LOGICAL-c561t-9cc6ea4b58fc26e2359d11a2084df69b269375cf1a99a110ef6cff2979f210573</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s11214-015-0175-6$$EPDF$$P50$$Gspringer$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s11214-015-0175-6$$EHTML$$P50$$Gspringer$$Hfree_for_read</linktohtml><link.rule.ids>314,776,780,27903,27904,41467,42536,51297</link.rule.ids></links><search><creatorcontrib>McFadden, J. P.</creatorcontrib><creatorcontrib>Kortmann, O.</creatorcontrib><creatorcontrib>Curtis, D.</creatorcontrib><creatorcontrib>Dalton, G.</creatorcontrib><creatorcontrib>Johnson, G.</creatorcontrib><creatorcontrib>Abiad, R.</creatorcontrib><creatorcontrib>Sterling, R.</creatorcontrib><creatorcontrib>Hatch, K.</creatorcontrib><creatorcontrib>Berg, P.</creatorcontrib><creatorcontrib>Tiu, C.</creatorcontrib><creatorcontrib>Gordon, D.</creatorcontrib><creatorcontrib>Heavner, S.</creatorcontrib><creatorcontrib>Robinson, M.</creatorcontrib><creatorcontrib>Marckwordt, M.</creatorcontrib><creatorcontrib>Lin, R.</creatorcontrib><creatorcontrib>Jakosky, B.</creatorcontrib><title>MAVEN SupraThermal and Thermal Ion Compostion (STATIC) Instrument</title><title>Space science reviews</title><addtitle>Space Sci Rev</addtitle><description>The MAVEN SupraThermal And Thermal Ion Compostion (STATIC) instrument is designed to measure the ion composition and distribution function of the cold Martian ionosphere, the heated suprathermal tail of this plasma in the upper ionosphere, and the pickup ions accelerated by solar wind electric fields. STATIC operates over an energy range of 0.1 eV up to 30 keV, with a base time resolution of 4 seconds. The instrument consists of a toroidal “top hat” electrostatic analyzer with a
360
∘
×
90
∘
field-of-view, combined with a time-of-flight (TOF) velocity analyzer with
22.5
∘
resolution in the detection plane. The TOF combines a
−
15
kV
acceleration voltage with ultra-thin carbon foils to resolve
H
+
,
He
+
+
,
He
+
,
O
+
,
O
2
+
, and
CO
2
+
ions. Secondary electrons from carbon foils are detected by microchannel plate detectors and binned into a variety of data products with varying energy, mass, angle, and time resolution. To prevent detector saturation when measuring cold ram ions at periapsis (
∼
10
1
1
eV/cm
2
s
sr
eV
), while maintaining adequate sensitivity to resolve tenuous pickup ions at apoapsis (
∼
10
3
eV/cm
2
s
sr
eV
), the sensor includes both mechanical and electrostatic attenuators that increase the dynamic range by a factor of
10
3
. This paper describes the instrument hardware, including several innovative improvements over previous TOF sensors, the ground calibrations of the sensor, the data products generated by the experiment, and some early measurements during cruise phase to Mars.</description><subject>Aerospace Technology and Astronautics</subject><subject>Analyzers (electric)</subject><subject>Astrophysics and Astroparticles</subject><subject>Carbon</subject><subject>Composting</subject><subject>Detectors</subject><subject>Electric fields</subject><subject>Electrostatics</subject><subject>Foils</subject><subject>Ionosphere</subject><subject>Ions</subject><subject>Mars</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Planetology</subject><subject>Sensors</subject><subject>Space exploration</subject><subject>Space Exploration and Astronautics</subject><subject>Space Sciences (including Extraterrestrial Physics</subject><subject>Spacecraft</subject><issn>0038-6308</issn><issn>1572-9672</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><sourceid>C6C</sourceid><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GNUQQ</sourceid><recordid>eNqNkMtKxDAUhoMoOI4-gLuCm3FRzUmb27IMXgqjLqa6DZlOojP0ZtIufHtTqiCC4OJwzuL7fzgfQueArwBjfu0BCKQxBhqG05gdoBlQTmLJODlEM4wTEbMEi2N04v0e4zHFZyh7yF5uHqP10DldvBlX6yrSzTb6vvO2iZZt3bW-34VzsS6yIl9eRnnjezfUpulP0ZHVlTdnX3uOnm9viuV9vHq6y5fZKi4pgz6WZcmMTjdU2JIwQxIqtwCaYJFuLZMbwmTCaWlBS6kBsLGstJZILi0BTHkyR4upt3Pt-2B8r-qdL01V6ca0g1fAucBYCC7-gVIgRHA2tl78Qvft4JrwSKBSSYXkXAYKJqp0rffOWNW5Xa3dhwKsRpNq8q-CfzX6VyxkyJTxgW1ejfvR_GfoE1eHhH8</recordid><startdate>20151201</startdate><enddate>20151201</enddate><creator>McFadden, J. P.</creator><creator>Kortmann, O.</creator><creator>Curtis, D.</creator><creator>Dalton, G.</creator><creator>Johnson, G.</creator><creator>Abiad, R.</creator><creator>Sterling, R.</creator><creator>Hatch, K.</creator><creator>Berg, P.</creator><creator>Tiu, C.</creator><creator>Gordon, D.</creator><creator>Heavner, S.</creator><creator>Robinson, M.</creator><creator>Marckwordt, M.</creator><creator>Lin, R.</creator><creator>Jakosky, B.</creator><general>Springer Netherlands</general><general>Springer Nature B.V</general><scope>C6C</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7TG</scope><scope>7XB</scope><scope>88I</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>GNUQQ</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>KL.</scope><scope>L7M</scope><scope>M2P</scope><scope>P5Z</scope><scope>P62</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>Q9U</scope></search><sort><creationdate>20151201</creationdate><title>MAVEN SupraThermal and Thermal Ion Compostion (STATIC) Instrument</title><author>McFadden, J. P. ; Kortmann, O. ; Curtis, D. ; Dalton, G. ; Johnson, G. ; Abiad, R. ; Sterling, R. ; Hatch, K. ; Berg, P. ; Tiu, C. ; Gordon, D. ; Heavner, S. ; Robinson, M. ; Marckwordt, M. ; Lin, R. ; Jakosky, B.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c561t-9cc6ea4b58fc26e2359d11a2084df69b269375cf1a99a110ef6cff2979f210573</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>Aerospace Technology and Astronautics</topic><topic>Analyzers (electric)</topic><topic>Astrophysics and Astroparticles</topic><topic>Carbon</topic><topic>Composting</topic><topic>Detectors</topic><topic>Electric fields</topic><topic>Electrostatics</topic><topic>Foils</topic><topic>Ionosphere</topic><topic>Ions</topic><topic>Mars</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Planetology</topic><topic>Sensors</topic><topic>Space exploration</topic><topic>Space Exploration and Astronautics</topic><topic>Space Sciences (including Extraterrestrial Physics</topic><topic>Spacecraft</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>McFadden, J. P.</creatorcontrib><creatorcontrib>Kortmann, O.</creatorcontrib><creatorcontrib>Curtis, D.</creatorcontrib><creatorcontrib>Dalton, G.</creatorcontrib><creatorcontrib>Johnson, G.</creatorcontrib><creatorcontrib>Abiad, R.</creatorcontrib><creatorcontrib>Sterling, R.</creatorcontrib><creatorcontrib>Hatch, K.</creatorcontrib><creatorcontrib>Berg, P.</creatorcontrib><creatorcontrib>Tiu, C.</creatorcontrib><creatorcontrib>Gordon, D.</creatorcontrib><creatorcontrib>Heavner, S.</creatorcontrib><creatorcontrib>Robinson, M.</creatorcontrib><creatorcontrib>Marckwordt, M.</creatorcontrib><creatorcontrib>Lin, R.</creatorcontrib><creatorcontrib>Jakosky, B.</creatorcontrib><collection>Springer Nature OA Free Journals</collection><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest One Sustainability</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection (ProQuest)</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>ProQuest Central Student</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Science Database</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central Basic</collection><jtitle>Space science reviews</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>McFadden, J. P.</au><au>Kortmann, O.</au><au>Curtis, D.</au><au>Dalton, G.</au><au>Johnson, G.</au><au>Abiad, R.</au><au>Sterling, R.</au><au>Hatch, K.</au><au>Berg, P.</au><au>Tiu, C.</au><au>Gordon, D.</au><au>Heavner, S.</au><au>Robinson, M.</au><au>Marckwordt, M.</au><au>Lin, R.</au><au>Jakosky, B.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>MAVEN SupraThermal and Thermal Ion Compostion (STATIC) Instrument</atitle><jtitle>Space science reviews</jtitle><stitle>Space Sci Rev</stitle><date>2015-12-01</date><risdate>2015</risdate><volume>195</volume><issue>1-4</issue><spage>199</spage><epage>256</epage><pages>199-256</pages><issn>0038-6308</issn><eissn>1572-9672</eissn><abstract>The MAVEN SupraThermal And Thermal Ion Compostion (STATIC) instrument is designed to measure the ion composition and distribution function of the cold Martian ionosphere, the heated suprathermal tail of this plasma in the upper ionosphere, and the pickup ions accelerated by solar wind electric fields. STATIC operates over an energy range of 0.1 eV up to 30 keV, with a base time resolution of 4 seconds. The instrument consists of a toroidal “top hat” electrostatic analyzer with a
360
∘
×
90
∘
field-of-view, combined with a time-of-flight (TOF) velocity analyzer with
22.5
∘
resolution in the detection plane. The TOF combines a
−
15
kV
acceleration voltage with ultra-thin carbon foils to resolve
H
+
,
He
+
+
,
He
+
,
O
+
,
O
2
+
, and
CO
2
+
ions. Secondary electrons from carbon foils are detected by microchannel plate detectors and binned into a variety of data products with varying energy, mass, angle, and time resolution. To prevent detector saturation when measuring cold ram ions at periapsis (
∼
10
1
1
eV/cm
2
s
sr
eV
), while maintaining adequate sensitivity to resolve tenuous pickup ions at apoapsis (
∼
10
3
eV/cm
2
s
sr
eV
), the sensor includes both mechanical and electrostatic attenuators that increase the dynamic range by a factor of
10
3
. This paper describes the instrument hardware, including several innovative improvements over previous TOF sensors, the ground calibrations of the sensor, the data products generated by the experiment, and some early measurements during cruise phase to Mars.</abstract><cop>Dordrecht</cop><pub>Springer Netherlands</pub><doi>10.1007/s11214-015-0175-6</doi><tpages>58</tpages><oa>free_for_read</oa></addata></record> |
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| ispartof | Space science reviews, 2015-12, Vol.195 (1-4), p.199-256 |
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| subjects | Aerospace Technology and Astronautics Analyzers (electric) Astrophysics and Astroparticles Carbon Composting Detectors Electric fields Electrostatics Foils Ionosphere Ions Mars Physics Physics and Astronomy Planetology Sensors Space exploration Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Spacecraft |
| title | MAVEN SupraThermal and Thermal Ion Compostion (STATIC) Instrument |
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