no more intrusion detection, replaced by open/close action when button push also adapted lights change scriptmaster
parent
0f425271f4
commit
68934624dd
9 changed files with 296 additions and 22 deletions
@ -0,0 +1,20 @@ |
||||
perl did not work |
||||
556 wget https://github.com/OpenLightingProject/libartnet/releases/download/1.1.2/libartnet-1.1.2.tar.gz |
||||
557 wget https://github.com/OpenLightingProject/artnet-examples/releases/download/0.3.13/artnet-examples-0.3.13.tar.gz |
||||
does not work with arduino (need reply on dmx node inquiry) |
||||
|
||||
git clone https://github.com/philchristensen/python-artnet.git |
||||
cd python-artnet/ |
||||
sudo python setup.py install |
||||
artnet script all_channels_full |
||||
ImportError: No module named cement.core |
||||
sudo easy_install setuptools_git |
||||
sudo easy_install bitstring |
||||
sudo easy_install cement |
||||
artnet script all_channels_full |
||||
# all lights are on, wow |
||||
artnet script all_channels_blackout |
||||
# all lights are off |
||||
sudo easy_install pip |
||||
sudo pip install pyyaml |
||||
|
||||
@ -0,0 +1,18 @@ |
||||
#!/bin/bash |
||||
# changes level2 state by the state of the main door |
||||
# i.e. people have to leave it open to keep status open |
||||
if [ "$1" = "pushed" ] && |
||||
[ "$(cat /run/spacestatus)" = "open" ] |
||||
then |
||||
FORM_action="close" /root/pidor/webserver/cgi-bin/pidor.sh |
||||
/root/pidor/scripts/upd_status.sh |
||||
fi |
||||
if [ "$1" = "released" ] && # if switch was released (the door opened, or someone is playing with the switch) |
||||
[ "$(cat /run/spacestatus)" = "closed" ] # the status was closed |
||||
# [ $(stat -c "%Y" /run/spacestatus) -lt $(date --date "1 hour ago" +%s) ] # since at least one hour |
||||
then |
||||
FORM_action="open" /root/pidor/webserver/cgi-bin/pidor.sh |
||||
/root/pidor/scripts/upd_status.sh |
||||
# echo "intrusion detected: space was closed since some time and locked, but now is still closed but unlocked" | wall |
||||
# logger -t $(basename $0) "INTRUSION ALARM. door was opened while status is closed" |
||||
fi |
||||
@ -1,8 +0,0 @@ |
||||
#!/bin/bash |
||||
if [ "$1" = "released" ] && # if switch was released (the door opened, or someone is playing with the switch) |
||||
[ "$(cat /run/spacestatus)" = "closed" ] && # the status was closed |
||||
[ $(stat -c "%Y" /run/spacestatus) -lt $(date --date "1 hour ago" +%s) ] # since at least one hour |
||||
then |
||||
echo "intrusion detected: space was closed since some time and locked, but now is still closed but unlocked" | wall |
||||
logger -t $(basename $0) "INTRUSION ALARM. door was opened while status is closed" |
||||
fi |
||||
@ -0,0 +1,231 @@ |
||||
#!/usr/bin/awk -f |
||||
# converted from C to awk by gunstick@syn2cat.lu 2014/10/02 |
||||
# based on http://www.sci.fi/~benefon/rscalc_cpp.html |
||||
# ugly C code gives ugly awk code, don't blame me |
||||
# input is like this: 49.5916 6.1407 2 |
||||
|
||||
# gawk program calculating the sunrise and sunset for |
||||
# the current date and a fixed location(latitude,longitude) |
||||
# Note, twilight calculation gives insufficient accuracy of results |
||||
# Jarmo Lammi 1999 - 2001 |
||||
# Last update July 21st, 2001 |
||||
|
||||
BEGIN { |
||||
|
||||
pi = 3.14159; |
||||
degs = 0.0; |
||||
rads = 0.0; |
||||
|
||||
L=g=daylen=0.0 |
||||
SunDia = 0.53; # Sunradius degrees |
||||
|
||||
AirRefr = 34.0 / 60.0; # athmospheric refraction degrees |
||||
} |
||||
# Get the days to J2000 |
||||
# h is UT in decimal hours |
||||
# FNday only works between 1901 to 2099 - see Meeus chapter 7 |
||||
|
||||
function FNday (y, m, d, h) { |
||||
luku = int(-7 * (y + (m + 9)/12)/4 + 275*m/9 + d); |
||||
# type casting necessary on PC DOS and TClite to avoid overflow |
||||
luku+= y*367; |
||||
return luku - 730531.5 + h/24.0; |
||||
}; |
||||
|
||||
# the function below returns an angle in the range |
||||
# 0 to 2*pi |
||||
|
||||
function FNrange ( x) { |
||||
b = 0.5*x / pi; |
||||
a = 2.0*pi * (b - int(b)); |
||||
if (a < 0) a = 2.0*pi + a; |
||||
return a; |
||||
}; |
||||
|
||||
# Calculating the hourangle |
||||
# |
||||
function f0( lat, declin) { |
||||
fo=dfo=0.0; |
||||
# Correction: different sign at S HS |
||||
dfo = rads*(0.5*SunDia + AirRefr) |
||||
if (lat < 0.0) { dfo = -dfo }; |
||||
fo = tan(declin + dfo) * tan(lat*rads); |
||||
if (fo>0.99999) { fo=1.0 }; # to avoid overflow // |
||||
fo = asin(fo) + pi/2.0; |
||||
return fo; |
||||
}; |
||||
|
||||
# Calculating the hourangle for twilight times |
||||
# |
||||
function f1(lat, declin) { |
||||
fi=df1=0.0; |
||||
# Correction: different sign at S HS |
||||
df1 = rads * 6.0; if (lat < 0.0) { df1 = -df1 }; |
||||
fi = tan(declin + df1) * tan(lat*rads); |
||||
if (fi>0.99999) { fi=1.0 } ; # to avoid overflow // |
||||
fi = asin(fi) + pi/2.0; |
||||
return fi; |
||||
}; |
||||
|
||||
|
||||
# Find the ecliptic longitude of the Sun |
||||
|
||||
function FNsun (d) { |
||||
|
||||
# mean longitude of the Sun |
||||
|
||||
L = FNrange(280.461 * rads + .9856474 * rads * d); |
||||
|
||||
# mean anomaly of the Sun |
||||
|
||||
g = FNrange(357.528 * rads + .9856003 * rads * d); |
||||
|
||||
# Ecliptic longitude of the Sun |
||||
|
||||
return FNrange(L + 1.915 * rads * sin(g) + .02 * rads * sin(2 * g)); |
||||
}; |
||||
|
||||
|
||||
# Display decimal hours in hours and minutes |
||||
function showhrmn( dhr) { |
||||
hr=mn=0; |
||||
hr= int(dhr); |
||||
mn = int((dhr - hr)*60); |
||||
|
||||
printf("%0d:%0d",hr,mn); |
||||
}; |
||||
|
||||
# awk misses some trigo functions |
||||
function asin(x) { return atan2(x, sqrt(1-x*x)) } |
||||
function tan(x) { return sin(x)/cos(x) } |
||||
{ |
||||
|
||||
y=m=day=h=latit=longit=0.0 |
||||
inlat=inlon=intz=0 |
||||
tzone=d=lambda=0 |
||||
obliq=alpha=delta=LL=equation=ha=hb=twx=0 |
||||
twam=altmax=noont=settm=riset=twpm=0 |
||||
sekunnit=0; |
||||
tm =0; |
||||
|
||||
degs = 180.0/pi; |
||||
rads = pi/180.0; |
||||
# get the date and time from the user |
||||
# read system date and extract the year |
||||
|
||||
# First get time **/ |
||||
sekunnit=systime(); |
||||
|
||||
# Next get localtime **/ |
||||
|
||||
#p=localtime(&sekunnit); |
||||
|
||||
y = strftime("%Y",sekunnit) # p->tm_year; |
||||
# this is Y2K compliant method |
||||
#y+= 1900; |
||||
m= strftime("%m",sekunnit) #m = p->tm_mon + 1; |
||||
|
||||
|
||||
day=strftime("%d",sekunnit) # day = p->tm_mday; |
||||
|
||||
h = 12; |
||||
|
||||
printf("year %4d month %2d\n",y,m); |
||||
printf("Input latitude, longitude [and timezone]\n"); |
||||
#scanf("%f", &inlat); scanf("%f", &inlon); |
||||
#scanf("%f", &intz); |
||||
inlat=$1 ; inlon=$2 |
||||
if($3 != "") { |
||||
intz=$3 |
||||
} else { # guess the timezone |
||||
intz=(systime()-mktime(strftime("%Y %m %d %H %M %S",systime(),1)))/3600 |
||||
} |
||||
latit = inlat; longit = inlon; |
||||
tzone = intz; |
||||
|
||||
# testing |
||||
# m=6; day=10; |
||||
|
||||
|
||||
d = FNday(y, m, day, h); |
||||
|
||||
# Use FNsun to find the ecliptic longitude of the |
||||
# Sun |
||||
|
||||
lambda = FNsun(d); |
||||
|
||||
# Obliquity of the ecliptic |
||||
|
||||
obliq = 23.439 * rads - .0000004 * rads * d; |
||||
|
||||
# Find the RA and DEC of the Sun |
||||
|
||||
alpha = atan2(cos(obliq) * sin(lambda), cos(lambda)); |
||||
delta = asin(sin(obliq) * sin(lambda)); |
||||
|
||||
# Find the Equation of Time |
||||
# in minutes |
||||
# Correction suggested by David Smith |
||||
LL = L - alpha; |
||||
if (L < pi) { LL += 2.0*pi } ; |
||||
equation = 1440.0 * (1.0 - LL / pi/2.0); |
||||
ha = f0(latit,delta); |
||||
hb = f1(latit,delta); |
||||
twx = hb - ha; # length of twilight in radians |
||||
twx = 12.0*twx/pi; # length of twilight in hours |
||||
printf "ha= %.2f hb= %.2f \n",ha,hb ; |
||||
# Conversion of angle to hours and minutes // |
||||
daylen = degs*ha/7.5; |
||||
if (daylen<0.0001) {daylen = 0.0;} |
||||
# arctic winter // |
||||
|
||||
riset = 12.0 - 12.0 * ha/pi + tzone - longit/15.0 + equation/60.0; |
||||
settm = 12.0 + 12.0 * ha/pi + tzone - longit/15.0 + equation/60.0; |
||||
noont = riset + 12.0 * ha/pi; |
||||
altmax = 90.0 + delta * degs - latit; |
||||
# Correction for S HS suggested by David Smith |
||||
# to express altitude as degrees from the N horizon |
||||
if (latit < delta * degs) altmax = 180.0 - altmax; |
||||
|
||||
twam = riset - twx; # morning twilight begin |
||||
twpm = settm + twx; # evening twilight end |
||||
|
||||
if (riset > 24.0) riset-= 24.0; |
||||
if (settm > 24.0) settm-= 24.0; |
||||
|
||||
print "\n sunrise and set"; |
||||
print "==============="; |
||||
|
||||
printf " year : %d \n",y ; |
||||
printf " month : %d \n",m ; |
||||
printf " day : %d \n\n",day ; |
||||
printf "Days since Y2K : %d \n",d; |
||||
|
||||
printf "Latitude : %3.1f, longitude: %3.1f, timezone: %3.1f \n",latit,longit,tzone ; |
||||
printf "Declination : %.2f \n",delta * degs ; |
||||
printf "Daylength : " ; showhrmn(daylen); printf " hours \n" ; |
||||
print "" |
||||
printf "Civil twilight: " ; |
||||
showhrmn(twam); |
||||
print "" |
||||
printf "Sunrise : " ; |
||||
showhrmn(riset); |
||||
printf " %d",mktime(strftime("%Y %m %d 00 00 00"))+int(riset*3600) |
||||
print "" |
||||
|
||||
printf "Sun altitude " ; |
||||
# Amendment by D. Smith |
||||
printf " %.2f degr",altmax ; |
||||
printf latit>=0.0 ? " South" : " North" ; |
||||
printf " at noontime " ; showhrmn(noont); ; |
||||
print "" |
||||
printf "Sunset : " ; |
||||
showhrmn(settm); |
||||
printf " %d",mktime(strftime("%Y %m %d 00 00 00"))+int(settm*3600) |
||||
print "" |
||||
printf "Civil twilight: " ; |
||||
showhrmn(twpm); print "" ; |
||||
print "" |
||||
|
||||
#return 0; |
||||
} |
||||
@ -0,0 +1,3 @@ |
||||
#!/bin/bash |
||||
echo "49.5916 6.1407" | $(dirname "$0")/rscalc.awk | |
||||
awk '/^Sunrise/{print $NF}' |
||||
@ -0,0 +1,3 @@ |
||||
#!/bin/bash |
||||
echo "49.5916 6.1407" | $(dirname "$0")/rscalc.awk | |
||||
awk '/^Sunset/{print $NF}' |
||||
Loading…
Reference in new issue