{"id":345,"date":"2022-09-23T20:52:33","date_gmt":"2022-09-23T17:52:33","guid":{"rendered":"https:\/\/baspik.com\/?page_id=345"},"modified":"2023-04-15T18:51:50","modified_gmt":"2023-04-15T15:51:50","slug":"space-research","status":"publish","type":"page","link":"https:\/\/baspik.com\/en\/applications\/space-research\/","title":{"rendered":"Space Research"},"content":{"rendered":"\n<div class=\"wp-block-cover alignfull is-position-bottom-center\" style=\"min-height:55vh;aspect-ratio:unset;\"><span aria-hidden=\"true\" class=\"wp-block-cover__background has-background-dim-0 has-background-dim\"><\/span><img loading=\"lazy\" decoding=\"async\" width=\"1440\" height=\"700\" class=\"wp-block-cover__image-background wp-image-2376\" alt=\"\" src=\"https:\/\/baspik.com\/en\/wp-content\/uploads\/sites\/5\/2023\/02\/big-space-research.webp\" data-object-fit=\"cover\" srcset=\"https:\/\/baspik.com\/en\/wp-content\/uploads\/sites\/5\/2023\/02\/big-space-research.webp 1440w, https:\/\/baspik.com\/en\/wp-content\/uploads\/sites\/5\/2023\/02\/big-space-research-300x146.webp 300w, https:\/\/baspik.com\/en\/wp-content\/uploads\/sites\/5\/2023\/02\/big-space-research-1024x498.webp 1024w, https:\/\/baspik.com\/en\/wp-content\/uploads\/sites\/5\/2023\/02\/big-space-research-768x373.webp 768w\" sizes=\"auto, (max-width: 1440px) 100vw, 1440px\" \/><div class=\"wp-block-cover__inner-container is-layout-flow wp-block-cover-is-layout-flow\">\n<div class=\"wp-block-group has-global-padding is-layout-constrained wp-block-group-is-layout-constrained\"><h1 class=\"with-text-shadow wp-block-post-title\">Space Research<\/h1><\/div>\n<\/div><\/div>\n\n\n\n<p class=\"is-style-emphasis has-primary-color has-text-color has-medium-font-size\">Microchannel plate photon counting detectors have been successfully used in a large number of space missions. Their advantages include high reliability, low power consumption, light weight, immunity to space radiation environment, solar blindness and high temporal and spatial resolution.<\/p>\n\n\n\n<div class=\"wp-block-group alignfull has-grey-10-background-color has-background has-global-padding is-layout-constrained wp-container-core-group-is-layout-71c63c14 wp-block-group-is-layout-constrained\" style=\"margin-top:var(--wp--preset--spacing--50);margin-bottom:0;padding-right:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--50);padding-left:var(--wp--preset--spacing--30)\">\n<h4 class=\"wp-block-heading\">International practices of the application of MCP detectors in space missions.<\/h4>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-28f84493 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<h6 class=\"wp-block-heading\">The <strong>All Sky Monitor M-2 <\/strong>(ASM M-2) project aboard the International Space Station for X-ray astronomy<\/h6>\n\n\n\n<p>The main idea of this <a href=\"https:\/\/tsniimash.ru\/science\/scientific-experiments-onboard-the-is-rs\/cnts\/experiments\/mvn_m_2\/\" data-type=\"URL\" data-id=\"https:\/\/tsniimash.ru\/science\/scientific-experiments-onboard-the-is-rs\/cnts\/experiments\/mvn_m_2\/\">project<\/a> is to create a planar detector based on silicon drift detectors, operating in the energy range of 1-30 keV. It is planned to use a collimator based on microchannel plates in order to limit the field of view of the instrument to 0.5-1 degrees.<\/p>\n<\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<h6 class=\"wp-block-heading\"><strong>Space-based scientific instruments developed at the Skobeltsyn Institute of Nuclear Physics, Moscow State University<\/strong><\/h6>\n\n\n\n<p>Secondary electron multiplier SEM 7B by VTC Baspik based on a microchannel plate assembly is used in the SKIF-HE integrated particle radiation spectrometer. The device is installed on 3 types of spacecraft:&nbsp; Meteor, Electro, Arktika 7, and is used for monitoring the state of the space environment such as solar proton flux, magnetosphere, geomagnetic disturbances and storms.<\/p>\n<\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-28f84493 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<h6 class=\"wp-block-heading\">Solar Probe Plus<\/h6>\n\n\n\n<figure class=\"wp-block-embed is-type-video is-provider-youtube wp-block-embed-youtube wp-embed-aspect-16-9 wp-has-aspect-ratio\"><div class=\"wp-block-embed__wrapper\">\n<iframe loading=\"lazy\" title=\"The Insane Engineering of the Parker Solar Probe\" width=\"500\" height=\"281\" src=\"https:\/\/www.youtube.com\/embed\/pOZhPz92Dic?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" referrerpolicy=\"strict-origin-when-cross-origin\" allowfullscreen><\/iframe>\n<\/div><\/figure>\n\n\n\n<p><strong><em>&nbsp;<\/em><\/strong>The NASA Integrated Science Investigation of the Sun (IS\u2609IS) instrument is designed to measure energetic electrons, protons and heavy ions.&nbsp;The instrument set includes two independent instruments: EPI-Hi and EPI-Lo for studying higher and lower energy particles.<\/p>\n\n\n\n<figure class=\"wp-block-image aligncenter size-medium\"><img decoding=\"async\" src=\"https:\/\/baspik.com\/wp-content\/uploads\/2022\/12\/solare-probe-1-300x175.webp\" alt=\"\" class=\"wp-image-1428\"\/><\/figure>\n\n\n\n<p>VTC Baspik in collaboration with the University of California produced a custom curved microchannel plate for the experimental design of the Parker Solar Probe.<\/p>\n\n\n\n<p><em>\u0418\u043d\u0444\u043e\u0440\u043c\u0430\u0446\u0438\u044f: <a rel=\"noreferrer noopener\" href=\"https:\/\/ntrs.nasa.gov\/api\/citations\/20110013395\/downloads\/20110013395.pdf\" target=\"_blank\">Solar Probe Plus<\/a><\/em><\/p>\n<\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<h6 class=\"wp-block-heading\">The scientific equipment set for studying transient atmospheric phenomena (TAP) in the UV and optical ranges<\/h6>\n\n\n\n<figure class=\"wp-block-embed is-type-video is-provider-youtube wp-block-embed-youtube wp-embed-aspect-16-9 wp-has-aspect-ratio\"><div class=\"wp-block-embed__wrapper\">\n<iframe loading=\"lazy\" title=\"\u041f\u043b\u0430\u043d\u0435\u0442\u0430 \u041a\u043e\u0440\u043e\u043b\u0451\u0432\u0430 \u2014 \u00ab\u0423\u0424 \u0430\u0442\u043c\u043e\u0441\u0444\u0435\u0440\u0430\u00bb\" width=\"500\" height=\"281\" src=\"https:\/\/www.youtube.com\/embed\/lXedBGVHc4o?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" referrerpolicy=\"strict-origin-when-cross-origin\" allowfullscreen><\/iframe>\n<\/div><\/figure>\n\n\n\n<p>The <a href=\"https:\/\/yandex.ru\/patents\/doc\/RU2711554C1_20200117\" data-type=\"URL\" data-id=\"https:\/\/yandex.ru\/patents\/doc\/RU2711554C1_20200117\">scientific equipment set for studying transient atmospheric phenomena (TAP) in the UV and optical ranges<\/a> includes a spatially sensitive spectrometer which is a small refracting telescope (SRT) with high temporal resolution for measuring the spectrum of optical radiation of TAP and lightning and an UV- and IR-radiation detector. The optical detector based on a microchannel plate provides detection of radiation in the range from far UV to soft X-rays.<\/p>\n<\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-28f84493 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<h6 class=\"wp-block-heading\">Spectrum-UV project<\/h6>\n\n\n\n<p>The <a href=\"https:\/\/www.laspace.ru\/company\/international-cooperation\/spectrum-uv\/\">Spectrum-UV project<\/a> creates unique scientific instruments designed for spectral observations of point objects in the range of 110-320 nm with high resolution (resolving power R &gt;50000). Such resolving power provides a detailed analysis of the physical and chemical properties of stars and other point sources. These functions in the Spectrum-UV project are performed by high-resolution VUVES and UVES spectrometers (vacuum ultraviolet echelle spectrometer and ultraviolet echelle spectrometer, respectively). The Vacuum Ultraviolet Echelle Spectrometer for use in the 110-176 nm spectral range includes microchannel plates. The Field Camera Unit (FCU) is one of the main scientific instruments of the Spectrum-UV project and is intended for obtaining high-quality direct images of space objects in the UV range using light filters, as well as for obtaining images in low-resolution field spectroscopy mode. Some of the main scientific tasks for which the FCU is designed are galaxy formation, Milky Way formation and evolution, physics of accretion and outflows, atmospheres of the Solar System planets and exoplanets, astrochemistry in the presence of strong UV radiation fields.<\/p>\n<\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<h6 class=\"wp-block-heading\">Longxia Yan-1 \u0438\u043b\u0438 Lobster Eye-1<\/h6>\n\n\n\n<figure class=\"wp-block-embed is-type-video is-provider-youtube wp-block-embed-youtube wp-embed-aspect-16-9 wp-has-aspect-ratio\"><div class=\"wp-block-embed__wrapper\">\n<iframe loading=\"lazy\" title=\"&quot;Lobsters&quot; in space - new x-ray telescopes + first 3 missions (Longxia Yan 1, SVOM, SMILE)\" width=\"500\" height=\"281\" src=\"https:\/\/www.youtube.com\/embed\/SZjjwiH5kH8?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" referrerpolicy=\"strict-origin-when-cross-origin\" allowfullscreen><\/iframe>\n<\/div><\/figure>\n\n\n\n<p><a href=\"https:\/\/www.researchgate.net\/publication\/362706239_Lobster_Eye_X-ray_Optics\" data-type=\"URL\" data-id=\"https:\/\/www.researchgate.net\/publication\/362706239_Lobster_Eye_X-ray_Optics\">Longxia Yan-1 or Lobster Eye-1<\/a>, also called Longxia Yan-X Shexian-1 or Lobster Eye X-Ray Exploration Satellite, is a small satellite designed to demonstrate the Lobster-Eye focused X-ray detector.&nbsp; Lobster Eye X-ray optics uses microchannel plates as a kind of X-ray equivalent of optical fibers to produce a wide field of X-ray sky images.<\/p>\n<\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-28f84493 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<h6 class=\"wp-block-heading\">Indo-Russian SING spectrometer project for installation aboard the Chinese modular space station (CSS)<\/h6>\n\n\n\n<p><a href=\"https:\/\/www.researchgate.net\/publication\/357356485_The_Indo-Russian_UV_Spectrograph_Project_for_the_Chinese_Space_Station_SING\" data-type=\"URL\" data-id=\"https:\/\/www.researchgate.net\/publication\/357356485_The_Indo-Russian_UV_Spectrograph_Project_for_the_Chinese_Space_Station_SING\">Indo-Russian SING spectrometer project<\/a> for installation aboard the Chinese modular space station (CSS). It consists of a long dumbbell slit and a flat holographic concave grid. The radiation detector is designed on the basis of microchannel plates.<\/p>\n<\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\"><\/div>\n<\/div>\n<\/div>\n\n\n\n<h4 class=\"wp-block-heading\">Product list:<\/h4>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-28f84493 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<div class=\"wp-block-group is-style-icon-box is-layout-flow wp-block-group-is-layout-flow\">\n<figure class=\"wp-block-image size-large box-icon\"><img decoding=\"async\" src=\"https:\/\/baspik.com\/wp-content\/uploads\/2022\/12\/icon-circle-mcp.svg\" alt=\"\" class=\"wp-image-1218\"\/><\/figure>\n\n\n\n<h5 class=\"wp-block-heading\"><a href=\"https:\/\/baspik.com\/en\/products\/microchannel-plates\/circular-mcps\/mcps-for-image-intensifier-tubes\/\" data-type=\"page\" data-id=\"701\">MCPs for Image Intensifier Tubes<\/a><\/h5>\n\n\n\n<ul class=\"bottom-small-text wp-block-list\">\n<li>Rimmed MCP 25-10A<\/li>\n<\/ul>\n<\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<div class=\"wp-block-group is-style-icon-box is-layout-flow wp-block-group-is-layout-flow\">\n<figure class=\"wp-block-image size-large box-icon\"><img decoding=\"async\" src=\"https:\/\/baspik.com\/wp-content\/uploads\/2022\/12\/icon-detectors-mcp.svg\" alt=\"\" class=\"wp-image-1220\"\/><\/figure>\n\n\n\n<h5 class=\"wp-block-heading\"><a href=\"https:\/\/baspik.com\/en\/products\/microchannel-plates\/circular-mcps\/detector-type-mcps\/\" data-type=\"page\" data-id=\"705\">Detector Type MCPs<\/a><\/h5>\n\n\n\n<div class=\"wp-block-columns is-not-stacked-on-mobile bottom-small-text is-layout-flex wp-container-core-columns-is-layout-28f84493 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<ul class=\"wp-block-list\">\n<li>Rimmed MCP 50-10<\/li>\n\n\n\n<li>Rimmed MCP 56-15<\/li>\n<\/ul>\n<\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<ul class=\"wp-block-list\">\n<li>Rimmed MCP 70-15<\/li>\n\n\n\n<li>Rimmed MCP 87-12<\/li>\n<\/ul>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-28f84493 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<div class=\"wp-block-group is-style-icon-box is-layout-flow wp-block-group-is-layout-flow\">\n<figure class=\"wp-block-image size-large box-icon\"><img decoding=\"async\" src=\"https:\/\/baspik.com\/wp-content\/uploads\/2022\/12\/icon-square-mcp.svg\" alt=\"\" class=\"wp-image-1217\"\/><\/figure>\n\n\n\n<h5 class=\"wp-block-heading\"><a href=\"https:\/\/baspik.com\/en\/products\/microchannel-plates\/rectangular-mcps\/\" data-type=\"page\" data-id=\"707\">Rectangular MCPs<\/a><\/h5>\n\n\n\n<ul class=\"bottom-small-text wp-block-list\">\n<li>MCP 54\u00d754<\/li>\n\n\n\n<li>MCP 100\u00d7100<\/li>\n<\/ul>\n<\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<div class=\"wp-block-group is-style-icon-box is-layout-flow wp-block-group-is-layout-flow\">\n<figure class=\"wp-block-image size-large box-icon\"><img decoding=\"async\" src=\"https:\/\/baspik.com\/wp-content\/uploads\/2022\/12\/icon-sem.svg\" alt=\"\" class=\"wp-image-1222\"\/><\/figure>\n\n\n\n<h5 class=\"wp-block-heading\"><a href=\"https:\/\/baspik.com\/en\/products\/detectors\/open-detectors\/detectors-for-quantitative-signal-measurement\/\" data-type=\"page\" data-id=\"638\">Detectors for Quantitative Dignal Measurement<\/a><\/h5>\n\n\n\n<ul class=\"bottom-small-text wp-block-list\">\n<li>SEM-7B<\/li>\n<\/ul>\n<\/div>\n<\/div>\n<\/div>\n","protected":false},"excerpt":{"rendered":"<p>Microchannel plate photon counting detectors have been successfully used in a large number of space missions. Their advantages include high reliability, low power consumption, light weight, immunity to space radiation environment, solar blindness and high temporal and spatial resolution. International practices of the application of MCP detectors in space missions. The All Sky Monitor M-2 [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":1561,"parent":133,"menu_order":5,"comment_status":"closed","ping_status":"closed","template":"wp-custom-template-stranicza-bez-zagolovka","meta":{"inline_featured_image":false,"footnotes":""},"tags":[],"class_list":["post-345","page","type-page","status-publish","has-post-thumbnail","hentry"],"_links":{"self":[{"href":"https:\/\/baspik.com\/en\/wp-json\/wp\/v2\/pages\/345","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/baspik.com\/en\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/baspik.com\/en\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/baspik.com\/en\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/baspik.com\/en\/wp-json\/wp\/v2\/comments?post=345"}],"version-history":[{"count":0,"href":"https:\/\/baspik.com\/en\/wp-json\/wp\/v2\/pages\/345\/revisions"}],"up":[{"embeddable":true,"href":"https:\/\/baspik.com\/en\/wp-json\/wp\/v2\/pages\/133"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/baspik.com\/en\/wp-json\/"}],"wp:attachment":[{"href":"https:\/\/baspik.com\/en\/wp-json\/wp\/v2\/media?parent=345"}],"wp:term":[{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/baspik.com\/en\/wp-json\/wp\/v2\/tags?post=345"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}