{"id":349,"date":"2026-10-21T01:27:52","date_gmt":"2026-10-21T06:27:52","guid":{"rendered":"https:\/\/radio.cvastro.org\/index.php\/build-a-radio-telescope\/"},"modified":"2026-10-21T01:27:52","modified_gmt":"2026-10-21T06:27:52","slug":"build-a-radio-telescope","status":"publish","type":"page","link":"https:\/\/radio.cvastro.org\/index.php\/build-a-radio-telescope\/","title":{"rendered":"Build a Radio Telescope"},"content":{"rendered":"\t<div class=\"cvas-site cvas-guide\" data-guide>\n\t\t<section class=\"guide-hero\"><div class=\"wrap\">\n\t\t\t<p class=\"eyebrow\">Build your own \u00b7 prices checked October 20, 2026<\/p>\n\t\t\t<h1>Build your own radio telescope<\/h1>\n\t\t\t<p class=\"lead\">You don't need a 20-foot dish to do real radio astronomy. Here are three ways in, all used by amateurs in the last two years: catch the Sun with an 18-inch TV dish, hear the hydrogen of the Milky Way, or start free with a telescope you control online.<\/p>\n\t\t\t<div class=\"g-live\">\n\t\t\t\t<div><span>The Sun in radio today<\/span><b class=\"g-flux\">\u2014<\/b><small class=\"g-flux-s\">Loading today's measurement\u2026<\/small><\/div>\n\t\t\t\t<div><span>Best time for the Sun today<\/span><b class=\"g-transit\">\u2014<\/b><small class=\"g-transit-s\"><\/small><\/div>\n\t\t\t\t<div><span>Milky Way straight overhead<\/span><b class=\"g-mw\">\u2014<\/b><small class=\"g-mw-s\"><\/small><\/div>\n\t\t\t<\/div>\n\t\t<\/div><\/section>\n\n\t\t<section class=\"g-tracks-sec\"><div class=\"wrap\">\n\t\t\t<div class=\"g-tracks\">\n\t\t\t\t<a class=\"g-track\" href=\"#sun\"><span class=\"g-tn\">1<\/span><h3>Sun Detector 2.0<\/h3><span class=\"bc-cost\">About $38 + a used TV dish<\/span><p>Detect the Sun at 12 GHz with a satellite dish and a USB radio. An afternoon to build; works in daylight.<\/p><\/a>\n\t\t\t\t<a class=\"g-track\" href=\"#hydrogen\"><span class=\"g-tn\">2<\/span><h3>Hear the Milky Way<\/h3><span class=\"bc-cost\">$88 to $375<\/span><p>Pick up the hydrogen line at 1420.4 MHz and measure how the galaxy turns. A kit, a horn, or a dish you build yourself.<\/p><\/a>\n\t\t\t\t<a class=\"g-track\" href=\"#free\"><span class=\"g-tn\">3<\/span><h3>Start free<\/h3><span class=\"bc-cost\">$0<\/span><p>Use a real radio telescope online, join a worldwide network, or follow a course before you buy anything.<\/p><\/a>\n\t\t\t<\/div>\n\t\t\t<div class=\"card g-sunbars\">\n\t\t\t\t<h3>How strongly each setup sees the Sun today<\/h3>\n\t\t\t\t<div class=\"g-bars\" aria-live=\"polite\"><p class=\"fine\">Waiting for today's solar measurement\u2026<\/p><\/div>\n\t\t\t\t<p class=\"fine g-bars-note\"><\/p>\n\t\t\t<\/div>\n\t\t<\/div><\/section>\n\n\t\t<section id=\"sun\"><div class=\"wrap\">\n\t\t\t<p class=\"eyebrow\">Track 1<\/p>\n\t\t\t<h2>Sun Detector 2.0<\/h2>\n\t\t\t<p class=\"lead-s\">Based on the <b>Itty Bitty Telescope<\/b>, designed by the late <b>Chuck Forster<\/b>, a CVAS member and a member of the Society of Amateur Radio Astronomers (SARA), and later improved by SARA member Kerry Smith. NRAO still uses it with schools. The original read the Sun on a satellite-finder meter; that meter (Channel Master 1004IF) is no longer made, so this version records the Sun on a computer with a $38 USB radio instead.<\/p>\n\t\t\t<div class=\"g-chain-wrap\" tabindex=\"0\" aria-label=\"Signal path diagram; scroll sideways on a small screen\"><svg class=\"g-chain\" viewBox=\"0 0 960 210\" role=\"img\" aria-label=\"Signal path: the dish focuses radio waves on the LNB; coax carries 950 to 1450 megahertz to a satellite power inserter that sends DC up the coax to the LNB; a DC block protects the USB radio, which connects to a laptop.\">\n\t\t\t\t<path d=\"M50 40 Q130 100 50 160\" class=\"gc-dish\"\/><line x1=\"50\" y1=\"100\" x2=\"132\" y2=\"100\" class=\"gc-arm\"\/>\n\t\t\t\t<rect x=\"132\" y=\"84\" width=\"54\" height=\"32\" rx=\"6\" class=\"gc-box\"\/><text x=\"159\" y=\"105\" class=\"gc-t\">LNB<\/text>\n\t\t\t\t<text x=\"92\" y=\"188\" class=\"gc-s\">18-inch TV dish<\/text>\n\t\t\t\t<line x1=\"186\" y1=\"100\" x2=\"300\" y2=\"100\" class=\"gc-coax\"\/><text x=\"243\" y=\"88\" class=\"gc-s\">950\u20131450 MHz<\/text>\n\t\t\t\t<rect x=\"300\" y=\"64\" width=\"150\" height=\"72\" rx=\"8\" class=\"gc-box\"\/><text x=\"375\" y=\"94\" class=\"gc-t\">Power inserter<\/text><text x=\"375\" y=\"114\" class=\"gc-s\">DC up the coax to the LNB<\/text>\n\t\t\t\t<line x1=\"375\" y1=\"136\" x2=\"375\" y2=\"172\" class=\"gc-wire\"\/><text x=\"375\" y=\"190\" class=\"gc-s\">wall power supply<\/text>\n\t\t\t\t<line x1=\"450\" y1=\"100\" x2=\"520\" y2=\"100\" class=\"gc-coax\"\/>\n\t\t\t\t<rect x=\"520\" y=\"80\" width=\"88\" height=\"40\" rx=\"6\" class=\"gc-box\"\/><text x=\"564\" y=\"105\" class=\"gc-t\">DC block<\/text>\n\t\t\t\t<line x1=\"608\" y1=\"100\" x2=\"668\" y2=\"100\" class=\"gc-coax\"\/>\n\t\t\t\t<rect x=\"668\" y=\"72\" width=\"120\" height=\"56\" rx=\"6\" class=\"gc-box\"\/><text x=\"728\" y=\"98\" class=\"gc-t\">USB radio<\/text><text x=\"728\" y=\"116\" class=\"gc-s\">RTL-SDR V4L<\/text>\n\t\t\t\t<line x1=\"788\" y1=\"100\" x2=\"840\" y2=\"100\" class=\"gc-wire\"\/>\n\t\t\t\t<rect x=\"840\" y=\"70\" width=\"100\" height=\"60\" rx=\"6\" class=\"gc-box\"\/><text x=\"890\" y=\"98\" class=\"gc-t\">Laptop<\/text><text x=\"890\" y=\"116\" class=\"gc-s\">logs the power<\/text>\n\t\t\t<\/svg><\/div>\n\t\t\t<p>The dish focuses radio waves onto the <b>LNB<\/b> (low-noise block converter), which amplifies the 12.2\u201312.7 GHz satellite band and shifts it down to 950\u20131450 MHz for ordinary coax (<a href=\"https:\/\/www.rtl-sdr.com\/rtl-sdr-based-itty-bitty-radio-telescope\/\">RTL-SDR.com<\/a>). The USB radio measures how much power arrives: anything warm in front of the dish raises it. The original Itty Bitty Telescope powered its LNB with 12 V from eight AA cells; satellite LNBs are normally fed 13 or 18 V up the coax, which a satellite <b>power inserter<\/b> does. The radio's own 4.5 V bias tee is too weak for an LNB, so leave it off, and the <b>DC block<\/b> keeps the LNB voltage out of the radio.<\/p>\n\t\t\t<div class=\"two\">\n\t\t\t\t<div>\n\t\t\t\t\t<h3>What you need<\/h3>\n\t\t\t\t\t<table class=\"g-table\">\n\t\t\t\t\t\t<tr><td>18-inch satellite TV dish with its LNB and mount<\/td><td>NRAO used a DirecTV 18-inch dish. Used ones are often free.<\/td><\/tr>\n\t\t\t\t\t\t<tr><td>RTL-SDR Blog V4L USB radio<\/td><td><b>$37.95<\/b> (rtl-sdr.com). Released August 2026 after the V4 sold out.<\/td><\/tr>\n\t\t\t\t\t\t<tr><td>Satellite power inserter with its supply<\/td><td>Puts 13\u201318 V on the coax for the LNB<\/td><\/tr>\n\t\t\t\t\t\t<tr><td>Inline DC block<\/td><td>Protects the radio from the LNB voltage<\/td><\/tr>\n\t\t\t\t\t\t<tr><td>75-ohm coax with F connectors, F-to-SMA adapter<\/td><td>The radio has an SMA socket<\/td><\/tr>\n\t\t\t\t\t\t<tr><td>75-ohm terminators<\/td><td>One for each unused LNB output<\/td><\/tr>\n\t\t\t\t\t\t<tr><td>A base that swivels<\/td><td>30 \u00d7 30 in board, a lazy Susan, screws and glue<\/td><\/tr>\n\t\t\t\t\t\t<tr><td>Laptop<\/td><td>Windows, Mac or Linux<\/td><\/tr>\n\t\t\t\t\t<\/table>\n\t\t\t\t<\/div>\n\t\t\t\t<div>\n\t\t\t\t\t<h3>Build it<\/h3>\n\t\t\t\t\t<ol class=\"g-steps\">\n\t\t\t\t\t\t<li><b>Make the base.<\/b> Centre the lazy Susan on the board, glue and screw it, and bolt the dish bracket to the turning top so the dish can swing and tilt. Make it heavy enough not to tip.<\/li>\n\t\t\t\t\t\t<li><b>Prepare the dish.<\/b> Put a 75-ohm terminator on every LNB output except one, and run coax from that output.<\/li>\n\t\t\t\t\t\t<li><b>Connect.<\/b> LNB coax \u2192 the inserter's dish\/LNB port; the inserter's receiver port \u2192 DC block \u2192 adapter \u2192 radio \u2192 laptop. Plug in the inserter.<\/li>\n\t\t\t\t\t\t<li><b>Install the software.<\/b> Follow the <a href=\"https:\/\/www.rtl-sdr.com\/QSG\">RTL-SDR quick-start guide<\/a> (the V4-series radios need the RTL-SDR Blog drivers). Turn automatic gain off and set a fixed gain.<\/li>\n\t\t\t\t\t\t<li><b>Log the power.<\/b> The free <code>rtl_power<\/code> tool writes power to a spreadsheet file every few seconds, for example <code>rtl_power -f 1150M:1250M:1M -i 2 -g 20 sun.csv<\/code>. Or watch the noise floor rise in SDR#.<\/li>\n\t\t\t\t\t<\/ol>\n\t\t\t\t<\/div>\n\t\t\t<\/div>\n\t\t\t<div class=\"two\">\n\t\t\t\t<div>\n\t\t\t\t\t<h3>Find the Sun<\/h3>\n\t\t\t\t\t<p class=\"warn\"><b>Never look at the Sun<\/b>, with or without anything in front of your eyes.<\/p>\n\t\t\t\t\t<ol class=\"g-steps\">\n\t\t\t\t\t\t<li><b>Read empty sky first.<\/b> Point at clear sky away from the Sun, trees and buildings. Note the power.<\/li>\n\t\t\t\t\t\t<li><b>Aim by shadow.<\/b> Turn and tilt until the LNB's shadow falls in the middle of the dish. The power rises as you get close.<\/li>\n\t\t\t\t\t\t<li><b>Peak it.<\/b> Small moves until the power is highest: you are on the Sun.<\/li>\n\t\t\t\t\t\t<li><b>Let the Earth turn.<\/b> Swing a little west of the Sun and leave it. The Sun drifts through in about <b class=\"g-drift-inline\">15 minutes<\/b> today, and your log shows a smooth hill.<\/li>\n\t\t\t\t\t<\/ol>\n\t\t\t\t<\/div>\n\t\t\t\t<div class=\"card physics\">\n\t\t\t\t\t<h3>Today's numbers for an 18-inch dish<\/h3>\n\t\t\t\t\t<ul>\n\t\t\t\t\t\t<li>Beam width at 12.45 GHz (2.41 cm): about <b>3.7\u00b0<\/b> (\u2248 70 \u03bb \/ D). The Sun is 0.53\u00b0 across.<\/li>\n\t\t\t\t\t\t<li>Sun's radio brightness at 12.45 GHz today: <b class=\"g-s12\">\u2014<\/b>, worked out from NOAA's measurements at 8.8 and 15.4 GHz.<\/li>\n\t\t\t\t\t\t<li>Signal the Sun adds: <b class=\"g-t12\">\u2014<\/b> (antenna temperature, T = \u03b7 A S \/ 2k with 50% efficiency).<\/li>\n\t\t\t\t\t\t<li>A tree or a person that fills the beam is about <b>300 K<\/b>, which is why the Itty Bitty manual notes trees read stronger than the Sun.<\/li>\n\t\t\t\t\t\t<li>Drift time today: <b class=\"g-drift\">\u2014<\/b>, at the Sun's declination of <span class=\"g-sdec\">\u2014<\/span>.<\/li>\n\t\t\t\t\t<\/ul>\n\t\t\t\t<\/div>\n\t\t\t<\/div>\n\t\t<\/div><\/section>\n\n\t\t<section id=\"hydrogen\" class=\"g-alt\"><div class=\"wrap\">\n\t\t\t<p class=\"eyebrow\">Track 2<\/p>\n\t\t\t<h2>Hear the Milky Way<\/h2>\n\t\t\t<p class=\"lead-s\">Cold hydrogen gas between the stars glows at <b>1420.4 MHz<\/b> (21 cm). Point a small dish or horn straight up and let the Earth turn: when the Milky Way passes overhead, the hydrogen appears as a bump in the spectrum, shifted by the gas's motion. IEEE Spectrum's David Schneider used those shifts from a homemade horn to <a href=\"https:\/\/www.rtl-sdr.com\/detecting-dark-matters-mark-with-an-rtl-sdr-based-diy-radio-telescope\/\">measure how the galaxy rotates<\/a>, matching professional results.<\/p>\n\t\t\t<div class=\"cards2\">\n\t\t\t\t<article class=\"card build-card\">\n\t\t\t\t\t<div class=\"bc-top\"><h3>Ready-made: Discovery Dish<\/h3><span class=\"bc-cost\">$311.95<\/span><\/div>\n\t\t\t\t\t<table class=\"g-table\">\n\t\t\t\t\t\t<tr><td>Discovery Dish, 70 cm (KrakenRF)<\/td><td>$149<\/td><\/tr>\n\t\t\t\t\t\t<tr><td>Hydrogen-line feed, amplifier and filter built in, 6 m coax<\/td><td>$125<\/td><\/tr>\n\t\t\t\t\t\t<tr><td>RTL-SDR Blog V4L (powers the feed through its bias tee)<\/td><td>$37.95<\/td><\/tr>\n\t\t\t\t\t\t<tr><td>Mast or tripod<\/td><td>your own<\/td><\/tr>\n\t\t\t\t\t<\/table>\n\t\t\t\t\t<p>Beam about <b class=\"g-dd-beam\">21\u00b0<\/b>; the Sun takes <b class=\"g-dd-drift\">\u2014<\/b> to drift through today. In February 2026 Dr. Kamal Jabbour <a href=\"https:\/\/www.crowdsupply.com\/krakenrf\/discovery-dish\/updates\/field-report-imaging-the-hydrogen-line-of-the-milky-way\">mapped the Milky Way's hydrogen<\/a> with one on a motorized mount, and caught a solar flare.<\/p>\n\t\t\t\t\t<a class=\"cvas-btn\" href=\"https:\/\/www.crowdsupply.com\/krakenrf\/discovery-dish\">Discovery Dish<\/a> <a class=\"cvas-btn cvas-btn-ghost\" href=\"https:\/\/github.com\/krakenrf\/discoverydish_docs\/wiki\/\">Setup guide<\/a>\n\t\t\t\t<\/article>\n\t\t\t\t<article class=\"card build-card\">\n\t\t\t\t\t<div class=\"bc-top\"><h3>Build it: horn or Wi-Fi grid dish<\/h3><span class=\"bc-cost\">$87.90 + antenna<\/span><\/div>\n\t\t\t\t\t<table class=\"g-table\">\n\t\t\t\t\t\t<tr><td>Nooelec SAWbird+ H1 amplifier + filter (40 dB gain, 0.8 dB noise figure)<\/td><td>$49.95<\/td><\/tr>\n\t\t\t\t\t\t<tr><td>RTL-SDR Blog V4L<\/td><td>$37.95<\/td><\/tr>\n\t\t\t\t\t\t<tr><td>Horn (aluminium flashing or foil board) or a 1 m Wi-Fi grid dish<\/td><td>see our <a href=\"https:\/\/radio.cvastro.org\/index.php\/2020\/03\/03\/newer-and-cheaper-amateur-radio-telescope\/\">club post<\/a><\/td><\/tr>\n\t\t\t\t\t<\/table>\n\t\t\t\t\t<p>A 1 m grid dish has a beam about <b class=\"g-grid-beam\">15\u00b0<\/b>. Tip: in December 2025 Alex P found the Discovery Dish feed on a 1 m Wi-Fi grid dish <a href=\"https:\/\/www.rtl-sdr.com\/discovery-dish-1420-mhz-hydrogen-line-feed-tested-with-a-wifi-grid-dish\/\">clearly beat<\/a> a standard feed with a separate amplifier.<\/p>\n\t\t\t\t\t<a class=\"cvas-btn\" href=\"https:\/\/www.nooelec.com\/store\/sawbird-h1.html\">SAWbird+ H1<\/a> <a class=\"cvas-btn cvas-btn-ghost\" href=\"https:\/\/www.rtl-sdr.com\/cheap-and-easy-hydrogen-line-radio-astronomy-with-a-rtl-sdr-wifi-parabolic-grid-dish-lna-and-sdrsharp\/\">Grid dish how-to<\/a>\n\t\t\t\t<\/article>\n\t\t\t<\/div>\n\n\t\t\t<div class=\"g-diy\" id=\"make-a-dish\">\n\t\t\t\t<h3>No dish? Make your own<\/h3>\n\t\t\t\t<p class=\"lead-s\">At 1420 MHz the radio waves are 21 cm (8.3 in) long, so a homemade dish does not need to be very precise. The SETI League's rules: the surface may stray up to a tenth of a wavelength (about <b>2 cm<\/b>) from the true curve, and mesh holes up to an eighth of a wavelength (about <b>2.6 cm<\/b>) still reflect well (<a href=\"https:\/\/setileague.org\/askdr\/accuracy.htm\">accuracy<\/a>, <a href=\"https:\/\/setileague.org\/askdr\/dishmesh.htm\">mesh<\/a>). That is woodworking accuracy.<\/p>\n\t\t\t\t<div class=\"g-diy-grid\">\n\t\t\t\t\t<div>\n\t\t\t\t\t\t<article class=\"card build-card g-diy-opt\">\n\t\t\t\t\t\t\t<div class=\"bc-top\"><h4>Simplest: a horn, no dish at all<\/h4><span class=\"bc-cost\">A weekend<\/span><\/div>\n\t\t\t\t\t\t\t<p>A pyramidal horn made of foil-covered foam board or aluminium flashing, with the SAWbird+ H1 and RTL-SDR at its back. Its beam is wider and the signal smaller than a dish's, but the Milky Way's hydrogen still shows up clearly.<\/p>\n\t\t\t\t\t\t\t<a href=\"https:\/\/radio.cvastro.org\/index.php\/2020\/03\/03\/newer-and-cheaper-amateur-radio-telescope\/\">Our club's horn post<\/a> \u00b7 <a href=\"https:\/\/www.rtl-sdr.com\/horn-antenna-rtl-sdr-radio-astronomy\/\">RTL-SDR.com horn antenna<\/a>\n\t\t\t\t\t\t<\/article>\n\t\t\t\t\t\t<article class=\"card build-card g-diy-opt\">\n\t\t\t\t\t\t\t<div class=\"bc-top\"><h4>Build a dish: ribs and wire mesh<\/h4><span class=\"bc-cost\">A few weekends<\/span><\/div>\n\t\t\t\t\t\t\t<ol class=\"g-steps\">\n\t\t\t\t\t\t\t\t<li><b>Pick a size<\/b> in the calculator. It prints the curve for your ribs.<\/li>\n\t\t\t\t\t\t\t\t<li><b>Cut 8 to 12 ribs<\/b> from plywood or aluminium flat bar. Mark each height from the table, join the marks with a flexible strip of wood, and cut along it.<\/li>\n\t\t\t\t\t\t\t\t<li><b>Mount the ribs<\/b> on a round hub like bicycle spokes, and tie their tips together with a rim ring so the shape can't twist.<\/li>\n\t\t\t\t\t\t\t\t<li><b>Cover with \u00bd-inch hardware cloth<\/b> (1.27 cm holes, well under the 2.6 cm limit). Fasten it to every rib with zip ties or rivets, overlap the seams and keep it tight.<\/li>\n\t\t\t\t\t\t\t\t<li><b>Make the feed<\/b> from a metal can or 6-inch duct with an end cap (sizes in the calculator), and hold it at the focus on three struts, its open end facing the dish.<\/li>\n\t\t\t\t\t\t\t\t<li><b>Anchor it.<\/b> A dish is a sail: bolt the mount down before the first windy day.<\/li>\n\t\t\t\t\t\t\t<\/ol>\n\t\t\t\t\t\t<\/article>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t<div class=\"card g-calc\" data-diy>\n\t\t\t\t\t\t<h4>Dish and feed calculator<\/h4>\n\t\t\t\t\t\t<div class=\"g-calc-in\">\n\t\t\t\t\t\t\t<label>Dish diameter<span><input type=\"number\" id=\"diy-d\" min=\"2\" max=\"20\" step=\"0.5\" value=\"6\" inputmode=\"decimal\"> ft<\/span><\/label>\n\t\t\t\t\t\t\t<label>Depth (focal ratio f\/D)<select id=\"diy-fd\"><option value=\"0.35\">0.35 (deep)<\/option><option value=\"0.4\" selected>0.40<\/option><option value=\"0.45\">0.45<\/option><option value=\"0.5\">0.50 (shallow)<\/option><\/select><\/label>\n\t\t\t\t\t\t\t<label>Feed can inside diameter<span><input type=\"number\" id=\"diy-can\" min=\"3\" max=\"9\" step=\"0.1\" value=\"6\" inputmode=\"decimal\"> in<\/span><\/label>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t\t\t<svg class=\"g-calc-fig\" viewBox=\"0 0 520 230\" role=\"img\" aria-label=\"Cross-section of the dish with its focus and feed\"><\/svg>\n\t\t\t\t\t\t<dl class=\"g-calc-out\"><\/dl>\n\t\t\t\t\t\t<h5>Rib heights (measured up from the centre of the dish)<\/h5>\n\t\t\t\t\t\t<div class=\"g-calc-tbl\"><\/div>\n\t\t\t\t\t\t<h5>Feed can<\/h5>\n\t\t\t\t\t\t<dl class=\"g-calc-feed\"><\/dl>\n\t\t\t\t\t\t<p class=\"fine\">Parabola: height = r\u00b2 \u00f7 (4 \u00d7 focal length). Beam \u2248 70 \u03bb\/D; gain and Sun signal assume 50% efficiency. Can limits are where the circular waveguide carries only its first mode (TE11 starts at \u03bb\/1.706, TM01 at \u03bb\/1.306). Probe position is a quarter of the guide wavelength from the closed end; where the focus sits inside the can uses the <a href=\"https:\/\/sites.science.oregonstate.edu\/~hetheriw\/astro\/rt\/info\/rf_antennas\/feedchok.htm\">SETI League feed formula<\/a>, whose 1420 MHz feed is 15.6 cm wide with a 4.6 cm probe 8.8 cm from the back.<\/p>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t<\/div>\n\n\t\t\t<div class=\"two g-radios\">\n\t\t\t\t<div>\n\t\t\t\t\t<h3>Which radio? RTL-SDR or Airspy Mini<\/h3>\n\t\t\t\t\t<table class=\"g-table g-cmp\">\n\t\t\t\t\t\t<tr><th><\/th><th>RTL-SDR Blog V4L<\/th><th>Airspy Mini<\/th><\/tr>\n\t\t\t\t\t\t<tr><td>Price<\/td><td>$37.95<\/td><td>$99 (Airspy store) to $165<\/td><\/tr>\n\t\t\t\t\t\t<tr><td>Hydrogen-line sensitivity<\/td><td colspan=\"2\" class=\"g-same\">The same: behind a 40 dB amplifier the radio adds under 0.2 K of noise<\/td><\/tr>\n\t\t\t\t\t\t<tr><td>Spectrum seen at once<\/td><td>2.4 MHz \u00b7 \u00b1253 km\/s<\/td><td>about 5 MHz \u00b7 \u00b1528 km\/s<\/td><\/tr>\n\t\t\t\t\t\t<tr><td>Converter<\/td><td>8-bit<\/td><td>12-bit, better with strong interference<\/td><\/tr>\n\t\t\t\t\t\t<tr><td>Clock<\/td><td>1 ppm (0.30 km\/s)<\/td><td>0.5 ppm (0.15 km\/s)<\/td><\/tr>\n\t\t\t\t\t\t<tr><td>Powers the amplifier?<\/td><td>Yes, 4.5 V bias tee<\/td><td>4.5 V but only 50 mA: power the SAWbird (120 mA) from its USB port<\/td><\/tr>\n\t\t\t\t\t<\/table>\n\t\t\t\t\t<p class=\"fine\">Start with the RTL-SDR. Step up to the Airspy Mini for wider, cleaner baselines and smoother drift scans (1.4\u20131.6\u00d7 less noise in the same time). Sources: <a href=\"https:\/\/airspy.com\/airspy-mini\/\">Airspy<\/a>, <a href=\"https:\/\/airspy.com\/quickstart\/\">Airspy quick start<\/a>, <a href=\"https:\/\/www.nooelec.com\/store\/sawbird-h1.html\">Nooelec<\/a>.<\/p>\n\t\t\t\t<\/div>\n\t\t\t\t<div>\n\t\t\t\t\t<h3>Observe it<\/h3>\n\t\t\t\t\t<ol class=\"g-steps\">\n\t\t\t\t\t\t<li><b>Point straight up<\/b> on a mast with a clear view, away from Wi-Fi routers and cell towers.<\/li>\n\t\t\t\t\t\t<li><b>Record a reference.<\/b> Average a few minutes of spectrum on empty sky (or with the feed covered) to subtract later.<\/li>\n\t\t\t\t\t\t<li><b>Average and watch.<\/b> With the Milky Way overhead, the hydrogen bump rises near 1420.4 MHz. Tonight's best times are at the top of this page.<\/li>\n\t\t\t\t\t\t<li><b>Free software:<\/b> SDR# with the IF Average plugin (Windows), <a href=\"https:\/\/github.com\/0xCoto\/Virgo\">Virgo<\/a> (open source), <a href=\"https:\/\/github.com\/tedcline\/ezRA\">ezRA<\/a> (open source), or GNU Radio.<\/li>\n\t\t\t\t\t<\/ol>\n\t\t\t\t<\/div>\n\t\t\t<\/div>\n\t\t<\/div><\/section>\n\n\t\t<section id=\"free\"><div class=\"wrap\">\n\t\t\t<p class=\"eyebrow\">Track 3<\/p>\n\t\t\t<h2>Start free<\/h2>\n\t\t\t<div class=\"cards3\">\n\t\t\t\t<article class=\"card\"><span class=\"card-k\">Online telescope<\/span><h3>PICTOR<\/h3><p>A 1.5 m radio telescope (1300\u20131700 MHz) that anyone can use free over the web, including for the hydrogen line.<\/p><a href=\"https:\/\/pictortelescope.com\/\">pictortelescope.com \u2192<\/a><\/article>\n\t\t\t\t<article class=\"card\"><span class=\"card-k\">Worldwide network<\/span><h3>WOW@Home<\/h3><p>A worldwide network of small hydrogen-line stations that check each other's detections, so local interference can be ruled out.<\/p><a href=\"https:\/\/phl.upr.edu\/wow\/outreach\">WOW@Home \u2192<\/a><\/article>\n\t\t\t\t<article class=\"card\"><span class=\"card-k\">Course<\/span><h3>SETI Institute ARISE<\/h3><p>Radio astronomy lessons and a lab for community colleges, launched in 2025.<\/p><a href=\"https:\/\/www.seti.org\/education\/arise\/\">ARISE \u2192<\/a><\/article>\n\t\t\t\t<article class=\"card\"><span class=\"card-k\">20 MHz<\/span><h3>NASA Radio JOVE<\/h3><p>Hear radio storms on Jupiter and the Sun with a wire antenna. The current kit (2.1) uses an SDRplay RSP1B radio.<\/p><a href=\"https:\/\/radiojove.gsfc.nasa.gov\/kits\/\">Radio JOVE kits \u2192<\/a><\/article>\n\t\t\t\t<article class=\"card\"><span class=\"card-k\">Community<\/span><h3>SARA<\/h3><p>The Society of Amateur Radio Astronomers: beginner booklet, mailing list and meetings. Chuck Forster's society too.<\/p><a href=\"https:\/\/www.radio-astronomy.org\/\">radio-astronomy.org \u2192<\/a><\/article>\n\t\t\t\t<article class=\"card\"><span class=\"card-k\">Ours<\/span><h3>Watch our 20-foot dish<\/h3><p>Our hydrogen-line data from Hobbs Observatory goes on the web as it is recorded.<\/p><a href=\"https:\/\/radio.cvastro.org\/index.php\/radio-telescope\/\">Live telescope \u2192<\/a><\/article>\n\t\t\t<\/div>\n\t\t<\/div><\/section>\n\n\t\t<section class=\"g-alt\"><div class=\"wrap two\">\n\t\t\t<div>\n\t\t\t\t<h2>Bring it to Hobbs<\/h2>\n\t\t\t\t<p>Built one? Stuck? Bring it to a work day and test it beside our 20-foot dishes, or send us a message.<\/p>\n\t\t\t\t<p><a class=\"cvas-btn cvas-btn-primary\" href=\"https:\/\/radio.cvastro.org\/index.php\/work-days\/\">Work days<\/a> <a class=\"cvas-btn\" href=\"https:\/\/radio.cvastro.org\/#join\">Contact us<\/a><\/p>\n\t\t\t<\/div>\n\t\t\t<div>\n\t\t\t\t<h3>Where these facts come from<\/h3>\n\t\t\t\t<p class=\"fine\">Prices from the sellers' own pages on October 20, 2026 (<a href=\"https:\/\/www.rtl-sdr.com\/product\/rtl-sdr-blog-v4l-lite-r828s-rtl2832u-1ppm-tcxo-sma-software-defined-radio-dongle-only\/\">RTL-SDR Blog<\/a>, <a href=\"https:\/\/www.crowdsupply.com\/krakenrf\/discovery-dish\">Crowd Supply<\/a>, <a href=\"https:\/\/www.nooelec.com\/store\/sawbird-h1.html\">Nooelec<\/a>, <a href=\"https:\/\/itead.cc\/product\/airspy-mini\/\">Airspy store<\/a>, <a href=\"https:\/\/pileupdx.com\/product\/airspy-mini\/\">PileupDX<\/a>); prices change. Itty Bitty Telescope: <a href=\"https:\/\/www.gb.nrao.edu\/epo\/ibt.shtml\">NRAO Green Bank<\/a>, <a href=\"https:\/\/www.aoc.nrao.edu\/epo\/teachers\/ittybitty\/procedure.html\">NRAO procedure<\/a>, <a href=\"https:\/\/www.gb.nrao.edu\/epo\/ambassadors\/ibtmanualshort.pdf\">IBT manual<\/a>, <em>Sky &amp; Telescope<\/em> March 2025. Solar flux: <a href=\"https:\/\/www.swpc.noaa.gov\/\">NOAA SWPC<\/a> from the US Air Force Radio Solar Telescope Network, updated daily. Beam widths use 70 \u03bb\/D; Sun signals assume 50% dish efficiency.<\/p>\n\t\t\t<\/div>\n\t\t<\/div><\/section>\n\t<\/div>\n\t\n","protected":false},"excerpt":{"rendered":"","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"cvas-full","meta":{"footnotes":""},"class_list":["post-349","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/radio.cvastro.org\/index.php\/wp-json\/wp\/v2\/pages\/349","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/radio.cvastro.org\/index.php\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/radio.cvastro.org\/index.php\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/radio.cvastro.org\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/radio.cvastro.org\/index.php\/wp-json\/wp\/v2\/comments?post=349"}],"version-history":[{"count":0,"href":"https:\/\/radio.cvastro.org\/index.php\/wp-json\/wp\/v2\/pages\/349\/revisions"}],"wp:attachment":[{"href":"https:\/\/radio.cvastro.org\/index.php\/wp-json\/wp\/v2\/media?parent=349"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}