
在本版中:AMSAT第44届年度研讨会亮点纷呈
* 2026年AMSAT-UK国际空间研讨会亮点
* 业余无线电卫星的65年历史
* 由学生自行组装的立方体卫星被发射升空,用于测试开源无线电技术和星间通信技术
AMSAT的负责人任命了三位新的志愿者网络大使。
* Meteor 使用MSK144在6米范围内进行散射通信
AMSAT CubeSatSim为2026年版本带来了许多令人兴奋的新功能。2026年10月16日,AMSAT卫星传输时间表的变更通知
* 阿里斯新闻
* AMSAT大使活动
来自AMSAT新闻服务各分站的卫星短讯,是AMSAT——业余无线电卫星公司提供的免费每周新闻信息服务。该网站发布与太空中的业余无线电相关的新闻,包括关于一群全球业余无线电操作员的活动的报道,这些操作员都热衷于设计、制造、发射模拟和数字式业余无线电卫星,并通过这些卫星进行通信。
在https://www.amsat.org上的新闻推送栏目会及时发布与太空业余无线电相关的新闻,这些新闻一旦由我们的志愿者们完成报道后就会立即被发布出来。
如果您有关于业余卫星的新闻或报道,请发送至:ans-editor [at] amsat.org。您可以通过ANS列表免费订阅AMSAT新闻服务的电子报;如需加入该列表,请访问:https://mailman.amsat.org/postorius/lists/ans.amsat.org/
AMSAT第44届年度研讨会[图片来源:AMSAT]
AMSAT在佛罗里达州的杰克逊维尔举办了第44届年度空间研讨会。会议内容涵盖了卫星操作、工程技术、教育培训以及未来任务规划等方面。周五安排了以教育为主题的专题演讲;周六则包含了技术方面的报告,同时举行了AMSAT的年度大会。与会者分享了当前项目的进展情况,并讨论了如何进一步推广太空业余无线电通信的发展。
AMSAT的主席德鲁·格拉斯布伦纳在年度股东大会上发表了讲话。他讨论了关于低地球轨道以外卫星任务的计划。AMSAT正在组建一个高轨道委员会,以制定任务方案并提出相关硬件需求。他们将整理出一系列未来任务思路,这些想法可以用于共享发射或搭载载荷等机会。格拉斯布伦纳强调,产业界与学术界之间的合作至关重要。
该活动的重点在于吸引更多学生和新志愿者加入。AMSAT希望这些学生能在未来的研讨会上展示他们的卫星相关研究成果。此外,他们还指出,25岁以下的学生可以免费成为会员。
CubeSat模拟器、GOLF、Fox-Plus计划更新:
在周五的活动中,AMSAT的CubeSat模拟器项目是一项非常重要的教育活动。该模拟器允许学生和业余操作者使用价格合理且易于使用的硬件来练习卫星通信操作。此外,AMSAT还与ARRL教师学院合作,在三个夏季课程中提供了超过30套模拟器设备供学生使用。
周六的工程会议主要讨论了GOLF和Fox-Plus卫星节目的更新事宜。Jerry Buxton介绍了GOLF-T项目的进展情况,而Fox-Plus项目则正在接近发射准备阶段。AMSAT的官员们正在评估政府支持和商业化的发射方案,以确保未来能够顺利发射这些卫星。这些卫星项目旨在推动空间技术的发展,同时为无线电爱好者提供更好的通信选择。
AMSAT还介绍了其线性转发器模块项目,该项目为大学卫星团队提供通信载荷支持。该硬件设备包含一个30 kHz的线性转发器,具有2米的高频信号传输距离、70厘米的下行信号传输距离,以及1200波特率的BPSK遥测技术。参与项目的大学可以通过向AMSAT租用并运营这些业余无线电转发器来获得该设备。AMSAT计划扩大这种模块的产量,以增加轨道上的有效转发器数量。
那些无法参加周五的教育课程和周六的技术培训会议的朋友们,可以通过AMSAT-NA的YouTube频道观看这些会议的录像资料。
周五的会议视频:https://www.youtube.com/watch?v=gaTIb-RBVYU 周六的会议视频:https://www.youtube.com/watch?v=QW49Dt9hRZE 在AMSAT仍在收集论文并整理全天视频内容期间,那些希望随时查看演讲材料的观众可以访问以下链接获取相关信息:https://www.amsat.org/2026-amsat-symposium-papers-and-presentations/
[ANS感谢AMSAT-NA提供的上述信息。]
2026年AMSAT-UK国际空间研讨会于2026年10月10日至11日在米尔顿凯恩斯市的肯茨山公园举行。该研讨会的重点是探讨如何将业余无线电技术融入现代数字通信体系,并测试下一代卫星载荷的性能。
主要的展示和活动亮点包括:
那些无法参加会议的朋友们可以通过AMSAT-UK的YouTube频道观看周六和周日举行的会议录像,包括年度股东大会的录像。
周六的直播链接:https://youtube.com/live/WQy0CXqjp3M 周日直播链接:https://youtube.com/live/CS6i-xeDm7o
[ANS感谢AMSAT-UK和AMSAT-SM提供的上述信息。]
业余无线电卫星跟踪技术的发展已经经历了六十多年的历程。从早期的太空飞行阶段到如今的便携式操作方式,这项技术取得了许多重要的技术进步。两种典型的卫星接收方式展示了设备与技术的巨大变革。
奥斯卡1号通信卫星 [图片来源:美国国家航空航天博物馆]
在1961年12月,凯斯西储大学一群业余无线电爱好者共同努力,成功接收到了第一颗业余无线电卫星——OSCAR 1的信号。
车站运营工作由团队成员分工负责,以处理早期卫星跟踪任务中的手动操作需求。
团队成功接收到美国“OSCAR I”卫星发来的独特“HI HI”摩斯电码信号。
用于监控Canada-OSCAR 128的天线设置 [来源:AMSAT-Canada]
在2026年8月,爱德华王子岛上的一个便携式设备正在监测加拿大卫星CO-128/马莫特卫星的传输信号,其传输频率为145.875 MHz。
所使用的便携式野外工作站包括:
操作员用摩斯电码记录了呼号CQ DEVA7UVS的通信内容。在传输过程中,音频输出产生的噪音比声音还要多。附近的电力线路最初会导致信号出现干扰现象,但将手指放在天线的铝制主杆上后,这种干扰就消失了,使得DEVA7UVS的信号更容易被接收。
[ANS感谢AMSAT-Canada、John DeDourek(前任负责人)以及Brent Petersen,VY2/VE9EX和W1IY,感谢他们提供的上述信息。]
SpaceX的Falcon 9火箭搭载学生设计的立方卫星成功发射[图片来源:NASA]
在2026年10月13日,SpaceX的Falcon 9火箭将两颗由学生自行组装的立方体卫星发射到了国际空间站。这是NASA第35次商业补给任务的一部分。此次发射任务由NASA的CubeSat发射计划负责执行,该计划的牵头单位是加州波莫纳理工大学。此次发射旨在展示开源太空技术的能力,并支持业余无线电操作。
这两颗立方星属于开源的Pleiades Five/PROVES项目。
这两项学生任务都采用了开源的“动态中继技术”来进行卫星间的数据传输,该技术旨在实现卫星间的容错性。这次发射是在之前由学生们自行组装的三颗PROVES卫星(Alcyone、Atlas和Electra)成功发射的基础上进行的。
[ANS感谢NASA和CSLI提供上述信息。]

AMSAT大使计划负责人很高兴地宣布,即将新增三位AMSAT大使:

弗兰克·卡纳乌斯卡斯,N1UW,AMSAT大使兼发展副总裁。2024年RST HamFest活动[图片来源:AMSAT]
AMSAT Ambassadors are dedicated volunteers who represent AMSAT at local ham fests, maker fairs, and club meetings. In their roles, Ambassadors agree to attend at least one local event per year and mentor area radio amateurs looking to get started with satellite operations.
To support their outreach efforts, each Ambassador receives:
A custom AMSAT Ambassador callsign badge
A 3′ x 5′ AMSAT banner flag
An “FAQ” presentation binder designed for interactive demonstrations
The presentation binder includes visual aids explaining core concepts such as satellite types, orbital mechanics, tracking software, antenna configurations, Doppler shift compensation, and operating techniques. The binder’s front cover features a QR code that directs interested operators directly to beginner articles and getting-started resources.
The Ambassador Program is open to current AMSAT members residing in the United States. U.S. members interested in joining the program can contact volunteer@amsat.org.
[ANS thanks Bo Lowry, W4FCL, AMSAT Director – Ambassador Program, for the above information.]
Amateur radio operators looking to expand beyond traditional local or HF modes can use meteor scatter propagation to make contacts over distances from 400 to 2,000 kilometers. As Earth moves through space, millions of meteors enter the upper atmosphere at altitudes of 80 km to 120 km, creating short-lived ionized trails that reflect VHF radio signals. While activity in southern Africa has historically lagged compared to active regions in North America and Europe, techniques using modern digital modes make this propagation path highly accessible.
Because meteor trails persist for only milliseconds to a few seconds, traditional voice communication is generally impractical outside of major annual meteor showers (such as the Perseids or Geminids). Instead, operators use specialized digital protocols:
MSK144 (Minimum Shift Keying at 144 baud), designed specifically for efficient meteor scatter communications within software like WSJT-X.
Stations exchange short data bursts using synchronized 15-second transmit/receive intervals.
The primary calling frequency on the 6-meter band is 50.260 MHz.
Because meteors enter the atmosphere at random angles across a shared sky area, multiple stations can operate on the same frequency simultaneously without interfering with one another.
Perseids Meteor Shower [Credit: AMSAT-SA]
Setting up a station for MSK144 meteor scatter requires minimal specialized hardware:
A 50 MHz (6-meter) radio capable of moderate power (typically 50W to 100W, though higher power increases contact speed).
A horizontal directional antenna (such as a 5- to 7-element Yagi) is strongly recommended over a vertical antenna to properly spread the signal horizontally across the reflection zone.
A computer running WSJT-X connected via a USB interface for CAT control, audio input/output, and PTT timing. Accurate PC clock synchronization (via an internet time server like Dimension 4) is critical to maintain precise 15-second sequencing.
While meteor scatter occurs 24/7, success rates improve significantly in the early morning when atmospheric meteor activity peaks, or during dedicated annual shower windows.
Pings may be brief, and completing a full QSO can take several minutes or longer depending on trail density and geometry. Operators monitor real-time spotting via platforms like PSK Reporter to coordinate active sessions.
[ANS thanks AMSAT-SA and the Southern Africa VHF group for the above information.]
– Educational Relations, announced several significant upgrades to the CubeSatSim satellite simulator, expanding its capabilities for amateur radio enthusiasts, educators, and students. The new software releases, versions 2.2 and 2.3, make the low-cost, open-source simulator an even more versatile tool for learning about satellite communications.
CubeSatSim Kit [Credit: AMSAT]
One major addition is PacSat mode, which simulates a packet-radio satellite that can store and forward digital messages and files between ground stations. Users can practice uploading and downloading information, recreating the operations of actual amateur radio satellites.
Another improvement is simulated Doppler shift, which reproduces the changing radio frequency experienced as a satellite passes overhead. During a simulated ten-minute pass, the transmitted frequency changes by approximately 18 kHz, providing realistic training for satellite operators.
A new web-based Dashboard lets users configure and control CubeSatSim from a computer or smartphone. The added Wi-Fi hotspot eliminates the need for an existing wireless network.
Version 2.2 also introduced simulated equipment failures, allowing students to practice identifying satellite problems through telemetry analysis.
Built around a Raspberry Pi Zero 2, CubeSatSim.org provides complete construction plans, software, and documentation.
[ANS thanks Alan Johnston, KU2Y, AMSAT VP – Educational Relations for the above information.]
Two Line Elements or TLEs, often referred to as Keplerian elements or keps in the amateur community, are the inputs to the SGP4 standard mathematical model of spacecraft orbits used by most amateur tracking programs. Weekly updates are completely adequate for most amateur satellites. TLE bulletin files are updated daily in the first hour of the UTC day. New bulletin files will be posted immediately after reliable elements become available for new amateur satellites. More information may be found at https://www.amsat.org/keplerian-elements-resources/.
Bulletin format elements for all satellites of interest to radio amateurs. This file is updated at least every 24 hours.
Bare elements are derived from the bulletin, but contain no header or footer. These data are used as input to the AMSAT Pass Predictions page.
This week there are no additions or deletions to the AMSAT TLE distribution.
AMSAT is pleased to announce that modern forms of what are called General Perturbations data are being disseminated via modern formats including JSON, XML and KVN at https://newark192.amsat.org/gpdata/current/. The reason this change is being made is that we are running out of 5-digit catalog numbers and the TLE format is not viable for satellites launched after July of this year. See https://celestrak.org/NORAD/documentation/gp-data-formats.php for details.
These data are presently considered in beta test for the next two months while hosted on the test server newark192.amsat.org, and we are very open to community feedback at webmaster [at] amsat.org. Testers may experience outages and errors while we make improvements. We intend to put this into production on our main web server in July as we expect that satellites launched after this summer will require one of the new formats to accommodate longer object numbers. AMSAT will continue to publish TLE bulletins for satellites launched before July 2026 indefinitely.
[ANS thanks Joe Fitzgerald, KM1P, AMSAT Orbital Elements Manager, for the above information.]
Amateurs and others around the world may listen in on contacts between amateur radio operators at schools and astronauts and cosmonauts aboard the International Space Station. The downlink frequency on which to listen is 145.800 MHz worldwide.
+ Recently Completed Ecole Internationale PACA de Manosque, Manosque, France — direct via F4KKM
The ISS callsign was NA1SS
The scheduled crewmember was Joshua Kutryk, KJ5BFU The ARISS mentor is F6ICS
Contact was successful: Fri 2026-10-16 10:03 UTC Congratulations to the students of international school EIPACA, crew member Joshua Kutryk, KJ5BFU, and mentor F6ICS.
EcoTarium Science Center, Worcester, MA — telebridge via AB1OC
The ISS callsign was NA1SS.
The scheduled crewmember is Luke Delaney, KJ5PPF.
The ARISS mentor was AB1OC
Contact was successful: Thu 2026-10-15 15:28 UTC Congratulations to the students at EcoTarium Science Center, crew member Luke Delaney, KJ5PPF, and mentor AB1OC.
+ Upcoming Contacts No Upcoming Contacts.
Many times, a school makes a last-minute decision to do a Livestream or runs into a last-minute glitch requiring a change of the URL, but ARISS may not get the URL in time for publication. You can always check https://live.ariss.org/ to see if a school is Livestreaming.
As always, if there is an EVA, a docking, or an undocking, the ARISS radios are turned off as part of the safety protocol.
2026-10-14 Expedition 75 Series 34 “ARISS Hardware” Begins Thursday, October 22; time TBD
Concludes Sunday, October 25; time TBD
Images will be transmitted at 437.55 MHz (+/- Doppler shift), decode with Robot 36 mode, transmission 36 seconds on, two minutes off.
Submit your images to the SSTV gallery for event certificate.
SSTV Series 34 [Credit: Ariss.org]
The crossband repeater remains configured in the Columbus Module (145.990 MHz up {PL 67} & 437.800 MHz down). If a crewmember decides to pick up the microphone and turn up the volume, you may hear the crew member on the air—so keep listening, as you never know when activity might occur.
Kenwood D710GA in the Zvezda Service Module – Callsign RSØISS. Please note we’re still in the process of troubleshooting and testing this radio. APRS is currently active on 437.825 MHz. Feel free to check out status reports at https://ariss-usa.org/ARISS_APRS/.
HamTV in the Columbus Module (2395.00 MHz) is currently transmitting a test signal. For more information, visit the ARISS Ham TV Live site at https://live.ariss.org/hamtv/.
Note that all times are approximate. It is recommended that you do your own orbital prediction or start listening about 10 minutes before the listed time.
The latest information on the operation mode can be found at https://www.ariss.org/current-status-of-iss-stations.html The latest list of frequencies in use can be found at https://www.ariss.org/contact-the-iss.html [ANS thanks Charlie Sufana, AJ9N, one of the ARISS operation team mentors for the above information.]
AMSAT Ambassadors provide presentations, demonstrate communicating through amateur satellites, and host information tables at club meetings, hamfests, conventions, maker fairs, and other events.
AMSAT Ambassador Clint Bradford, K6LCS, says, “Think a 75-minute presentation on ‘working the easy satellites’ would be appropriate for your club or event? Let me know by emailing me at k6lcsclint [at] gmail [dot] com or calling me at 909-999-SATS (7287)!” Clint has NEVER given the same show twice: EACH of the 150+ presentations so far has been customized to its audiences.
November 14, 2026
Oro Valley Amateur Radio Club Marana Middle School 11285 W. Grier Rd.
Marana AZ https://www.tucsonhamradio.org/hamfest
N1UW For more information go to: https://www.amsat.org/ambassador/ [ANS thanks Bo Lowrey, W4FCL, Director – AMSAT Ambassador Program, for the above information.]

+ Five spacecraft are currently docked at the International Space Station after a SpaceX Dragon cargo capsule arrived on Thursday morning, delivering over 6,300 pounds of scientific experiments, crew supplies, and roll-out solar arrays. Station crew members have begun transferring critical biological research and preparing for upcoming spacewalks on Oct. 29 and Nov. 5 to install the new solar arrays, while Roscosmos cosmonauts completed robotics and spatial orientation studies. [ANS thanks NASA for the above information.] + Media representatives are invited to attend the Europa-Park Science Days from October 22–24, 2026, in Rust, Germany, featuring presentations, STEM activities, and media opportunities with ESA experts. Highlights on Thursday, October 22, include a keynote address and interview opportunities with German ESA astronaut Alexander Gerst, alongside talks by ESA directors and interactive exhibits spanning VR experiences, robotics, and planetary science models. [ANS thanks ESA for the above information.] + Using NASA’s Chandra X-ray Observatory, eROSITA, and LOFAR, scientists observed a merging galaxy cluster nicknamed the “treble clef” due to its distinct, music-note-shaped radio emission. Researchers report in Astronomy & Astrophysics that it was likely generated and amplified by a violent collision between two galaxy clusters. [ANS thanks Space.com for the above information.] + Scientists from the Indian Institute of Astrophysics (IIA) and international collaborators analyzed joint observations of solar coronal mass ejections (CMEs) captured by India’s Aditya-L1 and ESA’s Proba-3 satellites. By combining spectroscopic data from VELC aboard Aditya-L1 with imaging from ASPIICS on Proba-3, the cross-checked observations provided new insights into CME mass, density, thermal energy, and early-stage dynamics in the low solar corona. [ANS thanks The Hindu and ISRO for the above information.] + The Australian Space Agency and the Roo-ver Consortium unveiled the latest design model of “Roo-ver,” Australia’s first lunar rover, at the Queensland University of Technology’s Lunar Testbed and Space Lab during World Space Week on October 7, 2026. Scheduled to land at the lunar South Pole in 2030 aboard an Intuitive Machines lander under NASA’s Commercial Lunar Payload Services (CLPS) program, the semi-autonomous rover will collect and analyze regolith to support sustainable human exploration through the Artemis program. Designed to withstand extreme lunar temperature swings from -246°C to 121°C, the vehicle features homegrown Australian technology including specialized treaded wheels, thermal management systems, and tools to mitigate against lunar dust and radiation. [ANS thanks the Australian Space Agency for the above information.]
In addition to regular membership, AMSAT offers membership to:
Contact info [at] amsat.org for additional membership information.
73 and remember to help Keep Amateur Radio in Space!
This week’s ANS Editor, Vidya Gopalakrishnan, K4VGK ANS is a service of AMSAT, the Radio Amateur Satellite Corporation, 712 H Street NE, Suite 1653, Washington, DC 20002
AMSAT is a registered trademark of the Radio Amateur Satellite Corporation.
来源:AMSAT 业余卫星组织 原文:查看原文 (本文由本站自动翻译整理,版权归原作者及原发布机构所有,仅供学习交流,如涉版权请联系我们删除。)