kirubeltadesse

function callDSMalgorithm()
{
	saveResult= false;
	imageList = new Array();
	callTime  = new Date().getTime();
	var vertex = saveTableValue();
	var soilfunction=readcheckbox("soil function");
	var terrainatrribute=readcheckbox("terrain attribute");

	var clusterselect=document.getElementById("ClusterNumber");

kirubeltadesse

import sys

class Vertex:
    def __init__(self, node):
        self.id = node
        self.adjacent = {}
        # Set distance to infinity for all nodes
        self.distance = sys.maxint
        # Mark all nodes unvisited        
        self.visited = False  

kirubeltadesse

DEVICE     = atmega328p
CLOCK      = 9830400
PROGRAMMER = -c usbtiny -P usb
OBJECTS    = main.o
FUSES      = -U hfuse:w:0xd9:m -U lfuse:w:0xe0:m

# Fuse Low Byte = 0xe0   Fuse High Byte = 0xd9   Fuse Extended Byte = 0xff
# Bit 7: CKDIV8  = 1     Bit 7: RSTDISBL  = 1    Bit 7:
#     6: CKOUT   = 1         6: DWEN      = 1        6:
#     5: SUT1    = 1         5: SPIEN     = 0        5:

kirubeltadesse

// this is a ROS version of the standard "hello, swarmies"
// program

// this header defines the standard ROS classes.
#include<ros/ros.h>

int main(int argc, char **argv){
	// Initialize the ROS system.
	ros::init(argc, argv, "hello_swarmies");
	

kirubeltadesse

#include <ros/ros.h>
#include <tf/transform_broadcaster.h>

char host[128];
std::string rover_name;
std::string hostname;


int main(int argc, char** argv){
    gethostname(host, sizeof(host));

kirubeltadesse

// assume
// the value of r will be on px value 
// the value of c will be on px value 
// (r,c) are the coordinate value in px on the image itself
// if you assume the image coordinate have u and v direciton r will be the value on the u axis
// and c will be the value on the v axis
// include math.h, ros.h the function of tan and arctan can be found on those header
 
#include <ros/ros.h>
#include <math.h>