Download "ОПРЕЛЕНИЕ ПОПРАВКИ ГИРОКОМПАСА по солнцу/флотбардак"
%3Aformat(webp)%2Fi.ytimg.com%252Fvi_webp%252F1TQAK3JFRZM%252Fmaxresdefault.webp&w=1139&q=75)
Please wait. We're preparing links for easy ad-free video watching and downloading.
Similar videos from our catalog
%3Aformat(webp)%2Fi.ytimg.com%252Fvi_webp%252FFN81XHUQt7k%252Fmaxresdefault.webp&w=1139&q=75)
%3Aformat(webp)%2Fi.ytimg.com%252Fvi_webp%252FHHBDs-MX6xI%252Fmaxresdefault.webp&w=1139&q=75)
%3Aformat(webp)%2Fi.ytimg.com%252Fvi_webp%252FM_Wml1cKGOo%252Fmaxresdefault.webp&w=1139&q=75)
%3Aformat(webp)%2Fi.ytimg.com%252Fvi%252FSqHqpM_R63A%252Fsd2.jpg%253Fsqp%253D-oaymwEoCIAFEOAD8quKqQMcGADwAQH4AbYIgAKAD4oCDAgAEAEYZSBlKGUwDw%253D%253D%2526rs%253DAOn4CLAtXtM5hb9nQHdU2-UEvm5iZGbCLw&w=1139&q=75)
%3Aformat(webp)%2Fi.ytimg.com%252Fvi%252FUowxttfoeiU%252Fmaxresdefault.jpg&w=1139&q=75)
Video tags
Subtitles
Russian
00:00:04
noise here. We are undergoing repairs with the arrival of new00:00:07
systems in the fleet. The life of a navigator is00:00:10
naturally made easier.00:00:12
For this, in principle, you were all00:00:14
created to make life easier for a navigator.00:00:16
However, this difficulty has not00:00:18
diminished because every year00:00:21
old systems are usually forgotten,00:00:24
for example, how to use sixta, we00:00:26
probably already even an experienced captain00:00:29
probably already remember how to determine the correction00:00:32
by the sun or the stars by the stars, too,00:00:35
few people know and I, of course, was00:00:40
no exception and00:00:44
he asked me to work with the captain captain of the old school00:00:47
captain I had a question in mind: how00:00:48
to determine the correction for the sun,00:00:51
not everyone, of course, didn’t know their method, I was00:00:52
just interested and curious about how to00:00:55
find this information at first, I started00:01:00
digging for information and came across a00:01:03
book like my nautical astronomical00:01:07
yearbook00:01:08
in it, in general, by and large, for this purpose00:01:11
who has never picked up this book was00:01:14
not all new, natural00:01:16
there were a lot of questions but the question00:01:19
remained unfinished how to determine the00:01:21
gyrocompass correction and at sunrise I00:01:24
went to YouTube and looked at it in the00:01:27
search bar like it stuck and00:01:30
naturally I won’t plagiarize and that’s why00:01:33
I I’ll just upload his video of this00:01:37
man,00:01:38
I’ll give a link to the channel in the description on how to find00:01:42
this real lesson of his, how he did it all00:01:47
from start to finish, but for00:01:50
you, this video will appear right now,00:01:53
so the more competent00:01:56
specialists there are in the fleet, the00:01:58
safer the fleet will be specialists would be more competent00:02:02
in general, watch00:02:05
enjoy the video everyone bye00:02:13
hello00:02:15
today we will analyze how you can00:02:17
calculate the compass correction based on some00:02:22
astronomical observations determined00:02:24
to calculate the compass correction we need to00:02:28
understand just one value00:02:30
to determine this is the azimuth from a certain00:02:32
luminary of some kind - then in the sky, that is,00:02:35
azimuth is the local bearing to the luminary, this is00:02:39
exactly what we will find in order for00:02:41
you to use computer programs here in a large number of00:02:43
different ways,00:02:48
why we can talk in our00:02:49
next lesson, you can use00:02:51
various books, that is, with various00:02:56
methods00:02:57
from these books that first of all you00:02:59
will need it most of all you will need it00:03:02
nautical estuaries in Russian00:03:05
international astronomical yearbook00:03:08
such a book in it you will find all00:03:11
the information you need to calculate the00:03:13
compass correction to determine the00:03:16
position of the ship there for various00:03:18
purposes it is necessary first of all00:03:20
besides it you can also use00:03:23
tables azimuth altitudes00:03:27
is a slightly larger book about00:03:30
the size of a person, and it basically00:03:33
contains various declinations and azimuths, and00:03:37
for you, the first volume in the first00:03:39
contains calculations for00:03:43
certain stars, that is, from it you can00:03:44
very quickly calculate the azimuths you need00:03:47
for certain stars00:03:51
you can do it very quickly,00:03:55
besides the first volume there are also 2 3 and00:04:00
4 azimuth altitude tables there, but it is already00:04:04
divided by direct latitude,00:04:08
that is, what is the latitude of what place you00:04:11
are, but in it you can find the necessary ones for00:04:13
any luminary on any celestial object00:04:15
you are looking for00:04:20
altitude deviations in azimuth and so on, that is,00:04:23
that is, here are their three volumes up to 15 30 3000:04:27
and 45 from 45 to 60 degrees, respectively,00:04:31
there is south and north,00:04:35
but we will not 20 today in the wilds00:04:38
and invent something extra let's go00:04:41
the most with the path at hand, what00:04:43
is on every passage on any ship00:04:45
is the international astronomical00:04:47
yearbook00:04:48
nautica, let's take a little00:04:51
look at what is in it in general, something in this00:04:53
book is in the beginning here on the first00:04:57
pages you will find you with various00:04:59
amendments but we are needed there corrections00:05:01
for the sextant and when the position of the ship is determined there are00:05:04
all sorts of adjustments high and00:05:09
so on the calendar here are00:05:11
daily calculations of some00:05:16
luminaries this additional various00:05:18
tables at the end in addition00:05:19
in the middle of the book and a00:05:22
wonderful map of the starry sky00:05:23
which will be useful to you if you want to00:05:25
study the various constellations Well, and so00:05:30
on, that it will be needed first of all,00:05:32
this is the first section that00:05:34
goes, this is the main section between the family of the00:05:39
tragic yearbook, which00:05:41
lists the hour angle and declination for00:05:45
most celestial objects, that is, the00:05:48
clinical number and time of00:05:53
the hour and for the stars is always00:05:57
necessary for us. smart and on the most defined00:06:02
celestial beds there and more often00:06:03
used such as Venus Mars00:06:06
Jupiter Saturn00:06:07
as well as the sun and moon,00:06:10
radiations have already been calculated, that is, this is the00:06:15
very table that you will need, that00:06:17
is, you will begin your first calculations00:06:19
with it except here00:06:22
is a table of00:06:23
corrections to these values for calculation00:06:28
for each specific moment in time00:06:31
then for a minute for a certain00:06:32
second and additional correction, the00:06:36
very last thing you need in00:06:39
your calculations is the table, also the00:06:43
azimuth altitude, such an abbreviated form of00:06:45
techno below which we are with you we saw that00:06:50
you can use it to00:06:51
calculate everything very quickly, well, let’s start00:06:55
these cluster calculations, now we’re00:06:58
starting the calculation, let’s first00:07:00
write down the measurements we made ourselves,00:07:03
measuring the peeling taken from our00:07:07
gyrocompass, and write down all these initial00:07:10
positions, that is, we have today 19 000:07:18
3 13 our position at the time of removing00:07:23
the peeling was from 5 degrees 12 and 300:07:28
March and mine is 3555 and but there is00:07:38
we took bearing 276 10 degrees00:07:48
and our time by the way we didn’t add it here either it00:07:54
was 1746 17 463000:08:05
local time and we correct this with00:08:08
our correction there for the time, it turns out to be00:08:11
two hours, the difference between us is Greenwich, yes, to00:08:13
study the mimic time will be 1546 3000:08:20
responsibly, so this is our genre, take everything,00:08:24
that is, all the necessary data00:08:26
that we needed for00:08:28
the calculation, we have now00:08:30
written everything down with you that is, now let's start00:08:34
our calculations, first00:08:37
we turn to my pockets00:08:42
and find, accordingly, the date when we00:08:46
made the calculation, so we found it00:08:51
turns out we have March 19, as you can see, until00:08:56
March 19, 2013 and we go down here and00:09:01
look below at the table on the left00:09:02
side we always have . Aries00:09:05
is the00:09:07
clinical hour angle for all stars, as well as for00:09:11
Venus and Mars, and for Jupiter with Saturn,00:09:14
and00:09:15
also for the stars, calculations are immediately given00:09:19
for some specific00:09:21
most popular stars, and that is, and00:09:25
goes to the right side of the right side,00:09:27
we already have silence some we00:09:30
need this for the sun here we also have for the00:09:32
moon there are also here there are still calculations00:09:36
when they will rise and set in00:09:39
different places there latitudes and so on00:09:41
but we don’t need this now we go00:09:43
directly to our give and here on00:09:46
March 19 and on the time when we filmed the00:09:49
borderland ska property in time it00:09:51
was 15 hours, that is, we only need00:09:53
an hour, that is, on March 19 at 15:00 we write down00:09:58
this data, it turns out 4300:10:02
clinical hour angle00:10:06
moving the angle itself 1 is equal to 43 degrees00:10:10
0 5 and 0 and we take it from here also the tables00:10:17
next to each other say we have declinations if00:10:19
you look if you look at the top of00:10:21
the table at the top of the table yes we publish it00:10:25
first in Greek then comes the00:10:28
declinations so on the right we take these values that is00:10:30
about sorting the patina00:10:36
the hour angle and declinations we take from here00:10:40
the sign yes that is south and here you see it’s written00:10:43
022 and 83 it’s also written by itself 019 800:10:53
here’s degrees 19.8 that’s how00:10:57
we recorded this data,00:11:03
now we need to select a correction for00:11:05
minutes and seconds because the time00:11:08
when we were filming was 1546 37 a00:11:12
very important indicator is minutes and00:11:14
seconds because during00:11:17
astronomical observations there, every00:11:20
second, one might say, matters for every00:11:22
second there are five seconds, the00:11:23
position of some object in the sky00:11:27
changes very much, the difference can be00:11:28
quite large, half a degree, and00:11:31
so on, you will need exactly all the00:11:33
bad compass, therefore be sure to00:11:35
take these corrections into account and take your00:11:39
observations, you probably have time00:11:43
to take these corrections, we go to the00:11:47
end of the table00:11:49
who is not from this book and look at our00:11:53
page, apparently00:11:56
46, here we have a page here, as you00:12:01
can see, it goes for every minute of some kind - then a00:12:04
certain correction to00:12:05
take 46 minutes, we had 30 seconds for00:12:08
the sun for the sun and planets 46 minutes 3000:12:13
seconds and we rewrite this figure,00:12:15
that is, this is our correction for the00:12:18
graphic hour angle, it is00:12:21
equal to 11 11 degrees00:12:28
thirty-seven and a half minutes00:12:34
that is, a doctor, when literally over a00:12:36
short period of time in00:12:38
the market there was a strong change in the00:12:39
hour angle, so these corrections00:12:41
need to be taken into account tomorrow,00:12:43
then we also find another correction for the00:12:46
declination, we didn’t look at our00:12:51
tables when we calculated it right away, well, we00:12:52
’ll look below now on the same00:12:55
page we got stuck at night00:12:56
if another amendment for declinations00:12:58
is called here is a small one written arno00:13:02
us 10 that is, it is calculated once a day00:13:04
and it also needs to be00:13:06
taken into account00:13:08
contact the killer00:13:10
46 minutes here it is here we select it here is the00:13:14
table heading amendment in or accident00:13:18
and directly for the sun we need and00:13:20
select with a value of 10 the corrections themselves will be increased00:13:24
will be 08 recorded00:13:28
correction00:13:31
that is, we have 0.8 minutes eight00:13:38
tenths of minutes all now we carry out the00:13:42
calculations so it turns out here00:13:47
54 degrees 42 and 5 so and here we00:13:54
get zero degrees00:13:59
2600:14:01
walls are familiar to that is, we00:14:05
got the local hour angle and the00:14:08
corrected declination, yes, that is, by00:14:10
correction, this is the longest tire,00:14:22
yes, sorry, yes, there is a small mistake,00:14:24
this is what we got with you given by about the00:14:27
time correction to give its 3000:14:31
seconds of the graphic hour angle, yes, that00:14:33
is, this is how it turns out, I was a little00:14:35
mistaken, now we need to bring this00:14:38
to our local location, yes, that00:14:42
is, for this, in order to00:14:44
calculate this, we need to00:14:48
add our longitude, that is,00:14:52
add 35 degrees 55 and 000:14:57
that is, if yours is eastern, then00:15:00
we add the local western there and00:15:02
subtract accordingly, so in the end00:15:07
we get and how much we get so much 0 9000:15:11
degrees we are 37 and a half here00:15:16
and now, of course, we already get the00:15:18
local hour angle here is the place hour00:15:21
angle and declination but00:15:22
corrected accordingly, that is,00:15:24
we need these two basic quantities00:15:26
directly for specific00:15:29
calculations of00:15:30
azimuth and this is the local hour angle and00:15:32
declination with which we can00:15:34
continue our calculations using the table,00:15:37
so we will continue in the future we will need it00:15:42
with you from00:15:47
the hour angle and declination you need to00:15:49
get the azimuth with you in this book in00:15:54
mine with necessarily such protection of this and00:15:55
ambush reduction tails which00:15:57
we very quickly find here00:15:59
if anything is not clear to you, you can00:16:01
refer to this book here00:16:04
everything is explained in detail how is this00:16:05
calculated and here, even in addition to00:16:07
the azimuth, you also get the height of the00:16:10
luminary by the horizon; this is necessary if00:16:12
you want to determine the position of the vessel on00:16:16
some page; observations are00:16:20
not of interest to us now, so we00:16:21
simply cut off half of these calculations and go with00:16:24
you the fast way; we receive only00:16:26
the azimuth for this is what we need, well, in general,00:16:30
let's go directly to00:16:33
the table, and the first input data00:16:38
that we need to00:16:39
get the value defined there is00:16:45
our wide pay and our local00:16:48
hour angle, these are the ones that we began to00:16:51
write down here, and our latitude00:16:58
pay accordingly, that is the first00:17:04
value that we will need to get is00:17:05
something like a degrees to00:17:13
respectively degrees and the first00:17:18
component of the azimuth z1, this is00:17:22
how we find them, we go into the background table00:17:26
with our latitude 3500:17:34
so here we go up to 3500:17:37
years derived smile 35 degrees and00:17:40
Mitya from the parameters is a b and00:17:41
accordingly there is money for this and we really00:17:44
need a commission for our place hourly hot00:17:47
it is equal to 90 degrees you can be00:17:49
happy to see here we list00:17:51
vegetables and should not be listed with these00:17:55
degrees at the very bottom of the table leads00:17:58
us there are 90 degrees, so it goes to00:18:01
rinse 1:35 and 90 and rewrite00:18:05
the value and ours is equal to 50 50 b,00:18:13
respectively, 0 and z1 is also equal to 0,00:18:18
but we have such a special case00:18:20
[music]00:18:22
directly which is the following00:18:25
data that we need to learn00:18:27
based on these calculations, if you follow00:18:30
the instructions, we need to learn such a00:18:34
value as f degrees, we00:18:37
will need it in order to subsequently obtain the00:18:39
second component of the azimuth degrees,00:18:43
we00:18:44
equal the sum of b, which we just00:18:48
found with you, and the00:18:50
rounded value of the declination, and plus00:18:54
in the future, of course, we need to00:18:56
take into account what we have a sign, yes there is a plus00:18:58
or a minus, but you and I00:19:00
will look at that right now, let's start with the calculations,00:19:03
look at the slope, don't you see if00:19:05
the mood is how we determine the sign00:19:08
for the declination, if for the declination,00:19:10
let's for example, yes, and our latitude holes,00:19:13
giving then, accordingly, the declinations we have00:19:16
negative if we have a declination sign00:19:19
and our latitudes coincide there, let's00:19:22
say proud and north you then00:19:25
our declination sign will be positive in00:19:28
this case we have a negative00:19:30
declination sign, so we write it down, it turns out00:19:32
we have zero degrees b plus negative00:19:37
yes there are 20 degrees and 60 and in the end we00:19:44
get 359 degrees m39 and 4 something like this,00:19:54
having a value such as f00:20:01
and having just about f and having such a00:20:04
value of x degrees, we can now00:20:06
calmly get the second00:20:08
component of the azimuth quite calmly, that is,00:20:11
use that00:20:14
we already have the same table of azimuth altitudes with00:20:17
these values of 55 degrees and00:20:22
is equal to this 359 and there we round it up, in00:20:26
the end we already find the tables and come00:20:30
here with the value looking for 55 degrees 50 5500:20:41
degrees here we have and where the00:20:44
latitude was the nose is also a drop 55 degrees and00:20:48
we round the declination to the nearest00:20:51
whole number, we get zero degrees and00:20:53
rewrite the corresponding values with the00:20:57
following value00:20:58
z2 that is, we don’t need these h-ips00:21:02
anymore, if we calculated it00:21:03
ourselves instead of the ship’s position we00:21:07
would need the height this is not necessary, we take00:21:09
z2 thinly,00:21:10
then the value for two, in this case we00:21:12
get 90 degrees for 2 equals 9000:21:17
degrees,00:21:19
everything is correct, that is, we, in principle, have done the00:21:21
basic calculations, we have done this blues,00:21:23
we no longer need it, that is, this is my little book,00:21:26
great, we no longer we don’t need00:21:28
that is, based on these values, we can00:21:31
already calculate us ours we need and in00:21:34
winter z will be equal to z1 +00:21:40
take two which, accordingly, 0 plus 9000:21:44
90 will be equal to should Erika understand00:21:47
90 90 degrees yourself but not so long ago00:21:51
tell us here here the initial00:21:53
calculations were canceled 27600:21:56
and we have a concert for some reason it00:21:57
turns out to be 90 and all this is because all00:22:01
these calculations are gray tables built00:22:03
on a circular azimuth, that is, here the00:22:06
maximum value of the azimuth development00:22:08
impression can only be 18000:22:09
degrees, that is, we now need espasa of00:22:11
circular azimuth translate this into00:22:14
circular, that is, at the end to 36000:22:17
degree azimuth, how is this00:22:19
calculated here in this table, let's00:22:23
carry out of couple, you can also00:22:25
look at it, what if you and I have00:22:33
prey, yes, here we look at the gift for northern00:22:36
latitude for northern latitude00:22:37
if we have the local hour angle is less than00:22:40
one hundred and eighty then, accordingly, the final final00:22:43
azimuth is equal to 360 minus z, yes, that is, these00:22:48
calculations if it were for a different value of00:22:49
Tobago, it is for this that we00:22:52
apply our rules now, that is, since we have for this00:22:59
he paid very, very much for compliance with Mitya 09000:23:03
less than less than 300 less00:23:06
than 18000:23:07
then, respectively, z m will be equal to00:23:12
360 360 degrees minus 90 degrees,00:23:17
respectively 270 degrees, we have00:23:21
calculated in principle, here is our final00:23:24
answer, this is our final00:23:27
final figure up to 270 degrees, the difference00:23:31
in the future is, in principle, not00:23:33
very difficult we now need to subtract or add from00:23:35
our true position of the sun at00:23:38
the time of calculations00:23:41
depending on the circumstances of00:23:44
the situation if we add our well,00:23:48
as if to the place taken with them taken our00:23:52
taken our peeling and accordingly we00:23:54
will receive in a certain folder of the compass00:23:56
then like all these our calculations00:23:58
the final ones, I’ll ask the compass to write it down in a00:24:01
journal, how to write it all out, I’ll00:24:04
tell you about all this in our next lesson,00:24:08
we’ve come, you and I have done a lot of00:24:10
work, yes, you and I would consider it a00:24:13
newfound achievement, I’d look at the lesson again,00:24:14
and here’s how to make these notes in principle00:24:17
thoughts of hello lessons but00:24:20
thank you all for your attention00:24:22
until the next lessonDescription:
https://www.youtube.com/watch?v=ebjvMgTaAMU&t=1s - ссылка на оригинал видео видео https://vk.com/public142288408 - подписывайся на нашу группу в ВК
Preparing download options
* — If the video is playing in a new tab, go to it, then right-click on the video and select "Save video as..."
** — Link intended for online playback in specialized players
Questions about downloading video
How can I download "ОПРЕЛЕНИЕ ПОПРАВКИ ГИРОКОМПАСА по солнцу/флотбардак" video?
http://unidownloader.com/ website is the best way to download a video or a separate audio track if you want to do without installing programs and extensions.
The UDL Helper extension is a convenient button that is seamlessly integrated into YouTube, Instagram and OK.ru sites for fast content download.
UDL Client program (for Windows) is the most powerful solution that supports more than 900 websites, social networks and video hosting sites, as well as any video quality that is available in the source.
UDL Lite is a really convenient way to access a website from your mobile device. With its help, you can easily download videos directly to your smartphone.
Which format of "ОПРЕЛЕНИЕ ПОПРАВКИ ГИРОКОМПАСА по солнцу/флотбардак" video should I choose?
The best quality formats are FullHD (1080p), 2K (1440p), 4K (2160p) and 8K (4320p). The higher the resolution of your screen, the higher the video quality should be. However, there are other factors to consider: download speed, amount of free space, and device performance during playback.
Why does my computer freeze when loading a "ОПРЕЛЕНИЕ ПОПРАВКИ ГИРОКОМПАСА по солнцу/флотбардак" video?
The browser/computer should not freeze completely! If this happens, please report it with a link to the video. Sometimes videos cannot be downloaded directly in a suitable format, so we have added the ability to convert the file to the desired format. In some cases, this process may actively use computer resources.
How can I download "ОПРЕЛЕНИЕ ПОПРАВКИ ГИРОКОМПАСА по солнцу/флотбардак" video to my phone?
You can download a video to your smartphone using the website or the PWA application UDL Lite. It is also possible to send a download link via QR code using the UDL Helper extension.
How can I download an audio track (music) to MP3 "ОПРЕЛЕНИЕ ПОПРАВКИ ГИРОКОМПАСА по солнцу/флотбардак"?
The most convenient way is to use the UDL Client program, which supports converting video to MP3 format. In some cases, MP3 can also be downloaded through the UDL Helper extension.
How can I save a frame from a video "ОПРЕЛЕНИЕ ПОПРАВКИ ГИРОКОМПАСА по солнцу/флотбардак"?
This feature is available in the UDL Helper extension. Make sure that "Show the video snapshot button" is checked in the settings. A camera icon should appear in the lower right corner of the player to the left of the "Settings" icon. When you click on it, the current frame from the video will be saved to your computer in JPEG format.
What's the price of all this stuff?
It costs nothing. Our services are absolutely free for all users. There are no PRO subscriptions, no restrictions on the number or maximum length of downloaded videos.