Very Long Baseline Array

{{Short description|System of ten radio telescopes}}

{{Infobox observatory}}

The Very Long Baseline Array (VLBA) is a system of ten radio telescopes which are operated remotely from their Array Operations Center located in Socorro, New Mexico, as a part of the National Radio Astronomy Observatory (NRAO).{{Cite web|url=https://public.nrao.edu/news/vlba-returning-to-nrao/|title=VLBA Returning to NRAO, Getting Technical Upgrade|website=NRAO eNews|publisher=National Radio Astronomy Observatory|date=2018-10-24|access-date=2019-12-21}} These ten radio antennas work together as an array that forms the longest system in the world that uses very long baseline interferometry. The longest baseline available in this interferometer is about {{convert|8611|km|0|sp=us}}.

The construction of the VLBA began in February 1986 and it was completed in May 1993. The first astrometrical observation using all ten antennas was carried out on May 29, 1993.{{Cite web|first=Ellen|last=Bouton|url=https://www.nrao.edu/archives/Timeline/timeline.shtml|title=National Radio Astronomy Observatory Archives: NRAO Timeline|publisher=National Radio Astronomy Observatory|date=2019-01-02|access-date=2019-03-31}} The total cost of building the VLBA was about $85 million. The array is funded by the National Science Foundation, and costs about $10 million a year to operate.{{cite news |last1=Lacitis |first1=Erik |title=Seeking the universe from an apple orchard in Brewster |url=https://www.seattletimes.com/seattle-news/seeking-the-universe-from-an-apple-orchard-in-brewster/ |access-date=2018-10-20 |work=The Seattle Times |date=2010-04-28}}

Each receiver in the VLBA consists of a parabolic dish antenna 25 meters (82 feet) in diameter, along with its adjacent control building. This contains the supporting electronics and machinery for the receiver, including low-noise electronics, digital computers, data storage units, and the antenna-pointing machinery. Each of the antennas is about as tall as a ten-story building when the antenna is pointed straight up, and each antenna weighs about 218 metric tons (240 short tons).

File:VLBA Owens Valley.JPG]]

The signals from each antenna are recorded on a bank of approximately one-terabyte hard disc drives, and the information is time-stamped using atomic clocks. Once the disc drives are loaded with information, they are carried to the Pete V. Domenici Science Operations Center at the NRAO in Socorro. There, the information undergoes signal processing in a powerful set of digital computers that carry out the interferometry. These computers also make corrections for the rotation of the Earth, the slight shifts in the crust of the Earth over time, and other small measurement errors.

Observations by the VLBA

The Very Long Baseline Array usually makes radio observations at wavelengths from three millimeters to 90 centimeters, or in other words, at frequencies from 0.3 gigahertz to 96 gigahertz. Within this frequency range, the VLBA observes in eight different frequency bands that are useful for radio astronomy. The VLBA also makes observations in two narrow radio bands below one gigahertz that include spectral lines produced by bright maser emissions.

The VLBA radio telescopes are located at:

{{Location map+ | USA

| width = 400

| caption = VLBA locations (red) and HSA locations (blue) in the contiguous United States

| places =

{{Location map~ | USA

| label = Hancock

| position =

| mark = Locator_Dot.png

| lat_deg = 42.93362

| lon_deg = -71.98681

}}

{{Location map~ | USA

| label = North Liberty

| position =

| mark = Locator_Dot.png

| lat_deg = 41.77165

| lon_deg = -91.574133

}}

{{Location map~ | USA

| label = Fort Davis

| position =

| mark = Locator_Dot.png

| lat_deg = 30.635214

| lon_deg = -103.944826

}}

{{Location map~ | USA

| label = Los Alamos

| position =

| mark = Locator_Dot.png

| lat_deg = 35.7752887

| lon_deg = -106.2455897

}}

{{Location map~ | USA

| label = Pie Town

| position = left

| mark = Locator_Dot.png

| lat_deg = 34.30107

| lon_deg = -108.11912

}}

{{Location map~ | USA

| label = Kitt Peak

| position =left

| mark = Locator_Dot.png

| lat_deg = 31.956253

| lon_deg = -111.612361

}}

{{Location map~ | USA

| label = Owens Valley

| position =

| mark = Locator_Dot.png

| lat_deg = 37.23176

| lon_deg = -118.27714

}}

{{Location map~ | USA

| label = Brewster

| position =bottom

| mark = Locator_Dot.png

| lat_deg = 48.13117

| lon_deg = -119.68325

}}

{{Location map~ | USA

| label = Green Bank

| position =right

| mark = Location dot blue.svg

| lat_deg = 38.255924

| lon_deg = -79.502341

}}

{{Location map~ | USA

| label = VLA

| position = bottom

| mark = Location dot blue.svg

| lat_deg = 34.079643

| lon_deg = -107.370591

}}

}}

{{Location map+ | World

| width = 400

| caption = VLBA locations (red) and HSA locations (blue) around the world

| places =

{{Location map~ | World

| label = St. Croix

| position =

| mark = Locator_Dot.png

| lat_deg = 17.75652

| lon_deg = -64.58376

}}

{{Location map~ | World

| label = Mauna Kea

| position =

| mark = Locator_Dot.png

| lat_deg = 19.80159

| lon_deg = -155.45581

}}

{{Location map~ | World

| label = Effelsberg

| position =

| mark = Location dot blue.svg

| lat_deg = 50.3130

| lon_deg = 6.53003

}}

}}

class="wikitable"

|+VLBA Locations

!scope="col"| Toponym

!scope="col"| U.S. state

!scope="col"| Geographic coordinate system

|

----

!scope="row"| St. Croix

| U.S. Virgin Islands

| {{coord|17.75652

64.58376}}

| SC

----

!scope="row"| Hancock

| New Hampshire

| {{coord|42.93362

71.98681}}

| HN

----

!scope="row"| North Liberty

| Iowa

| {{coord|41.77165

91.574133}}

| NL

----

!scope="row"| Fort Davis

| Texas

| {{coord|30.635214

103.944826}}

| FD

----

!scope="row"| Los Alamos

| New Mexico

| {{coord|35.7752887

106.2455897}}

| LA

----

!scope="row"| Pie Town

| New Mexico

| {{coord|34.30107

108.11912}}

| PT

----

!scope="row"| Kitt Peak

| Arizona

| {{coord| 31.956253

111.612361}}

| KP

----

!scope="row"| Owens Valley

| California

| {{coord|37.23176

118.27714}}

| OV

----

!scope="row"| Brewster

| Washington

| {{coord|48.13117

119.68325}}

| BR

----

!scope="row"| Mauna Kea

| Hawaii

| {{coord|19.80159

155.45581}}

| MK

High-Sensitivity Array

The use of the VLBA can be scheduled dynamically, and its sensitivity can be improved by a factor of five by including other radio telescopes such as the Green Bank Telescope in West Virginia, the Very Large Array (VLA) in New Mexico and the Effelsberg radio telescope in Germany. These three additional sites are brought online for as much as 100 hours per four-month trimester. In this configuration, the entire array is known as the High-Sensitivity Array (HSA).{{cite web|url=https://science.nrao.edu/facilities/vlba/HSA|title=High Sensitivity Array -- Science Website|first1=Amy|last1=Mioduszewski|first2=Justin|last2=Linford|date=2020-12-01|publisher=National Radio Astronomy Observatory|url-status=live|archive-url=https://web.archive.org/web/20210124220136/https://science.nrao.edu/facilities/vlba/HSA|archive-date=2021-01-24}} The Arecibo radio telescope in Puerto Rico was also used, before it collapsed.

class="wikitable"

|+High-Sensitive Array locations

!scope="col"| Toponym

!scope="col"| State

!scope="col"| Geographic coordinate system

----

!scope="row"| Green Bank

| West Virginia

| {{coord|38|25|59|N|79|50|23|W}}

| GB

----

!scope="row"| Very Large Array

| New Mexico

| {{coord|34|04|44|N|107|37|06|W}}

| Y27

----

!scope="row"| Effelsberg

| Germany

| {{coord|50|31|30|N|6|53|00|E}}

| EB

Baseline distance and angular resolution

File:Radio Telescope at Mauna Kea.jpg]]

Distance between each VLBA baseline (km):{{cite web|title=8 Angular Resolution & u-v Coverage|url=http://www.vlba.nrao.edu/astro/obstatus/2012-01-06/node24.html|first=Jon|last=Romney|date=2012-01-05|publisher=National Radio Astronomy Observatory}}

class="wikitable" border="1"

|+Distances between locations

scope="col" style="text-align:center;"|—

!scope="col" style="text-align:center;"|{{abbr|SC|St. Croix}}

!scope="col" style="text-align:center;"|{{abbr|HN|Hancock}}

!scope="col" style="text-align:center;"|{{abbr|NL|North Liberty}}

!scope="col" style="text-align:center;"|{{abbr|FD|Fort Davis}}

!scope="col" style="text-align:center;"|{{abbr|LA|Los Alamos}}

!scope="col" style="text-align:center;"|{{abbr|PT|Pie Town}}

!scope="col" style="text-align:center;"|{{abbr|KP|Kitt Peak}}

!scope="col" style="text-align:center;"|{{abbr|OV|Owens Valley}}

!scope="col" style="text-align:center;"|{{abbr|BR|Brewster}}

!scope="col" style="text-align:center;"|{{abbr|MK|Mauna Kea}}

!scope="col" style="text-align:center;"|{{abbr|EB|Effelsberg}}

!scope="col" style="text-align:center;"|{{abbr|AR|Arecibo}}

!scope="col" style="text-align:center;"|{{abbr|GB|Green Bank}}

!scope="col" style="text-align:center;"|{{abbr|Y27|Very Large Array}}

scope="row"|SC

|style="text-align:center;"|—

|2853

|3645

|4143

|4458

|4579

|4839

|5460

|5767

|8611

|6822

|238

|2708

|4532

scope="row"|HN

|2853

|style="text-align:center;"|—

|1611

|3105

|3006

|3226

|3623

|3885

|3657

|7502

|5602

|2748

|829

|3198

scope="row"|NL

|3645

|1611

|style="text-align:center;"|—

|1654

|1432

|1663

|2075

|2328

|2300

|6156

|6734

|3461

|1064

|1640

scope="row"|FD

|4143

|3105

|1654

|style="text-align:center;"|—

|608

|564

|744

|1508

|2345

|5134

|8084

|3922

|2354

|515

scope="row"|LA

|4458

|3006

|1432

|608

|style="text-align:center;"|—

|236

|652

|1088

|1757

|4970

|7831

|4246

|2344

|226

scope="row"|PT

|4579

|3226

|1663

|564

|236

|style="text-align:center;"|—

|417

|973

|1806

|4795

|8014

|4365

|2551

|52

scope="row"|KP

|4839

|3623

|2075

|744

|652

|417

|style="text-align:center;"|—

|845

|1913

|4466

|8321

|4623

|2939

|441

scope="row"|OV

|5460

|3885

|2328

|1508

|1088

|973

|845

|style="text-align:center;"|—

|1214

|4015

|8203

|5255

|3323

|1025

scope="row"|BR

|5767

|3657

|2300

|2345

|1757

|1806

|1913

|1214

|style="text-align:center;"|—

|4398

|7441

|5585

|3326

|1849

scope="row"|MK

|8611

|7502

|6156

|5134

|4970

|4795

|4466

|4015

|4398

|style="text-align:center;"|—

|10328

|8434

|7028

|4835

scope="row"|EB

|6822

|5602

|6734

|8084

|7831

|8014

|8321

|8203

|7441

|10328

|style="text-align:center;"|—

|6911

|6335

|8008

scope="row"|AR

|238

|2748

|3461

|3922

|4246

|4365

|4623

|5255

|5585

|8434

|6911

|style="text-align:center;"|—

|2545

|4317

scope="row"|GB

|2708

|829

|1064

|2354

|2344

|2551

|2939

|3323

|3326

|7028

|6335

|2545

|style="text-align:center;"|—

|2516

scope="row"|Y27

|4532

|3198

|1640

|515

|226

|52

|441

|1025

|1849

|4835

|8008

|4317

|2516

|style="text-align:center;"|—

The longest baseline in the array is {{convert|8611|km|0}}.

class="wikitable" border="1"

|+Minimum angular resolution

scope="col"|Wavelength (cm)

!scope="col"|90

!scope="col"|50

!scope="col"|21

!scope="col"|18

!scope="col"|13

!scope="col"|6

!scope="col"|4

!scope="col"|2

!scope="col"|1

!scope="col"|0.7

scope="row"|\theta_{HPBW} (milliarcseconds)

|22

|12

|5.0

|4.3

|3.2

|1.4

|0.85

|0.47

|0.32

|0.17

See also

References

{{Reflist|refs=

{{citation | first1=Swapan Kumar | last1=Saha | title=Aperture Synthesis: Methods and Applications to Optical Astronomy | series=Astronomy and Astrophysics Library | publisher=Springer | year=2010 | isbn=978-1-4419-5709-2 | page=81 | url=https://books.google.com/books?id=BIHe2Mmv08cC&pg=PA81 }}

}}